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Spica, the bright beacon of Virgo, is 2 stars

Brilliant blue-white star Spica with 4 rays against star field.
Even though our eyes see the star Spica as 1 star, it’s really at least 2. Photo by Fred Espenak at AstroPixels. Used with permission.

Spica is a close double star

The star Spica – aka Alpha Virginis – is the brightest star in the constellation Virgo the Maiden. From our distance of about 250 light-years away, Spica appears as a lone blue-white star. But the single point of light we see as Spica is really at least two stars.

Both the stars that we know make up Spica are larger and hotter than our sun. And they’re separated by only 11 million miles (less than 18 million km). That’s not much more than 10% of the distance between Earth and our sun (93 million miles or 150 million km). They orbit their common center of gravity in only four days.

Because they’re so close, the two stars in the Spica system are individually indistinguishable from a single point of light, even with a telescope. Only the analysis of its light with a spectroscope – an instrument that splits light into its component colors – revealed the dual nature of this star.

Hot, hot, hot

Spica’s two stars are so close, and they orbit so quickly around each other, that their mutual gravity distorts each star into an egg shape. It’s thought that the pointed ends of these egg-shaped stars face each other as they whirl around.

The pair of stars are both dwarf stars, brightening as they near the end of their lifetimes.

Spica is one of the hottest 1st-magnitude star systems. The hottest of the pair is about 40,000 degrees F or 22,000 C. That’s blistering in contrast to the sun’s 10,000 F or 5,500 C. This star might someday explode as a supernova.

The light from Spica’s two stars, taken together, is on average more than 12,100 times brighter than our sun’s light. Their estimated diameters are 7.8 and 4 times our sun’s diameter.

Spica is one of several bright stars that the moon occasionally passes in front of. And that gives astronomers a great opportunity to study the star system closely. By observing precisely how Spica’s light is extinguished when the moon passes in front of it, some astronomers think that it may not just be a binary star. Instead, they think that there may be as many as three other stars in the system. So Spica might not be a double star, but a quintuple star!

How to find Spica from the Northern Hemisphere

Live in the Southern Hemisphere? Here’s how to see Spica.

The best evening views of Spica come from northern spring to late northern summer, when this star arcs across the southern sky in the evening. So in the month of May, as seen from the Northern Hemisphere, you’ll find Spica in the southeast in early evening. From the Southern Hemisphere, Spica will be closer to due east. From all of Earth in May, as night passes, Spica appears to move westward. Spica rises earlier each evening so that – by the end of August – it can be viewed only briefly in the west to west-southwest sky as darkness falls.

There’s a foolproof way to find Spica, using the Big Dipper as a guide. Scouts and stargazers remember this trick with the saying: Follow the arc to Arcturus, and speed on (or drive a spike) to Spica.

Look for the Big Dipper

First, look for the Big Dipper in the northern sky. It’s highest in the evening sky in the northern spring and summer. Notice that the Big Dipper has a bowl and a long, curved handle. Follow the arc of the Dipper’s handle outward, away from the Dipper’s bowl. The first bright star you come to is orange Arcturus. Then speed on (or drive a spike) along this curving path. And the next bright star you come to is Spica.

Spica shines at magnitude 1.04, making it the brightest light in Virgo. In fact, it’s the 15th-brightest star visible from anywhere on Earth. It’s virtually the same brightness as Antares in the constellation Scorpius, so sometimes Antares is listed as the 15th and Spica as the 16th brightest.

Kite shaped constellation with a tail pointing to a dot labeled Arcturus and then to another dot labeled Spica.
In northern spring, look northeast to southeast in the evening. You’ll find the Big Dipper in the northeast evening sky. Then, follow the arc to Arcturus, and speed on to Spica.
Star chart showing Big Dipper with line to Arcturus continuing to Spica.
In northern summer, look northwest to southwest. You’ll find the Big Dipper in the northwest evening sky. But you can still follow the arc to Arcturus, and drive a speed on to Spica.

History and mythology of Spica

The name Spica is from the Latin word for “ear” (of grain). The general connotation is that Spica refers to an “ear of wheat.” Indeed, the star and the constellation Virgo itself were sometimes associated with the Greek goddess of the harvest, Demeter.

There are many names and stories for Spica’s constellation – Virgo – in mythology, and by association with Spica as well. Fewer stories refer to Spica independently. Many classical references refer to Virgo’s stars as a goddess or with some association with wheat or the harvest, since the sun passes through Virgo in the fall. In Greece and Rome she typically was Astraea, the very personification of Justice; or Persephone, daughter of Demeter. In Egypt, Virgo was identified with Isis, and Spica was considered her lute bearer. In ancient China, Spica was a special star of spring known as the Horn.

One Arabic name was Azimech, derived from words meaning Defenseless One or Solitary One. This title may be in reference to Spica’s solitary status with no other bright stars nearby. But Spica is not the most solitary star. That honor goes to Fomalhaut, sometimes called the Autumn Star.

Antique colored etching of winged young woman in long dress holding a wheat ear, with labeled scattered stars.
Here’s a classical illustration of the constellation Virgo the Maiden, with Spica embedded in the wheat in her left hand. Image via Urania’s Mirror/ Wikipedia (public domain).

How to see Spica from the Southern Hemisphere

Via Daniel Gaussen, Founder & Guide – Stargaze Mackenzie – New Zealand

For Southern Hemisphere observers, Spica’s constellation Virgo is one of the most prominent constellations of the autumn evening sky during May and June. Instead of looking south as Northern Hemisphere observers do, Southern Hemisphere stargazers should look toward the northern sky, where Virgo crosses the meridian high above the horizon.

The constellation appears upside down compared with Northern Hemisphere star charts, a reminder that our view of the celestial sphere is reversed. Despite this different orientation, the bright blue-white star Spica remains easy to identify as Virgo’s brightest star.

One of the easiest ways to find Spica is by using the so-called Spring Triangle, formed by Spica, Arcturus, and Regulus. This was named for Northern Hemisphere spring, so it’s actually seen during autumn in the south. During May and June evenings, these three bright stars dominate the northern sky, with Spica reaching highest of the three.

For observers in New Zealand’s South Island (around 45 latitude south), Spica reaches an altitude of about 61° when crossing the meridian, while from Auckland (37 latitude south) it culminates around 53° above the northern horizon.

Look for the distinctive shape of Virgo extending below Spica. The constellation forms a large, somewhat rectangular pattern of stars, although these stars are much fainter than Virgo’s brightest star.

Bottom line: Spica is the brightest star in Virgo. Spica is at least two stars orbiting extremely close together, distorting each other into egg shapes.

Virgo the Maiden represents a harvest goddess

The post Spica, the bright beacon of Virgo, is 2 stars first appeared on EarthSky.



from EarthSky https://ift.tt/WplD6vz
Brilliant blue-white star Spica with 4 rays against star field.
Even though our eyes see the star Spica as 1 star, it’s really at least 2. Photo by Fred Espenak at AstroPixels. Used with permission.

Spica is a close double star

The star Spica – aka Alpha Virginis – is the brightest star in the constellation Virgo the Maiden. From our distance of about 250 light-years away, Spica appears as a lone blue-white star. But the single point of light we see as Spica is really at least two stars.

Both the stars that we know make up Spica are larger and hotter than our sun. And they’re separated by only 11 million miles (less than 18 million km). That’s not much more than 10% of the distance between Earth and our sun (93 million miles or 150 million km). They orbit their common center of gravity in only four days.

Because they’re so close, the two stars in the Spica system are individually indistinguishable from a single point of light, even with a telescope. Only the analysis of its light with a spectroscope – an instrument that splits light into its component colors – revealed the dual nature of this star.

Hot, hot, hot

Spica’s two stars are so close, and they orbit so quickly around each other, that their mutual gravity distorts each star into an egg shape. It’s thought that the pointed ends of these egg-shaped stars face each other as they whirl around.

The pair of stars are both dwarf stars, brightening as they near the end of their lifetimes.

Spica is one of the hottest 1st-magnitude star systems. The hottest of the pair is about 40,000 degrees F or 22,000 C. That’s blistering in contrast to the sun’s 10,000 F or 5,500 C. This star might someday explode as a supernova.

The light from Spica’s two stars, taken together, is on average more than 12,100 times brighter than our sun’s light. Their estimated diameters are 7.8 and 4 times our sun’s diameter.

Spica is one of several bright stars that the moon occasionally passes in front of. And that gives astronomers a great opportunity to study the star system closely. By observing precisely how Spica’s light is extinguished when the moon passes in front of it, some astronomers think that it may not just be a binary star. Instead, they think that there may be as many as three other stars in the system. So Spica might not be a double star, but a quintuple star!

How to find Spica from the Northern Hemisphere

Live in the Southern Hemisphere? Here’s how to see Spica.

The best evening views of Spica come from northern spring to late northern summer, when this star arcs across the southern sky in the evening. So in the month of May, as seen from the Northern Hemisphere, you’ll find Spica in the southeast in early evening. From the Southern Hemisphere, Spica will be closer to due east. From all of Earth in May, as night passes, Spica appears to move westward. Spica rises earlier each evening so that – by the end of August – it can be viewed only briefly in the west to west-southwest sky as darkness falls.

There’s a foolproof way to find Spica, using the Big Dipper as a guide. Scouts and stargazers remember this trick with the saying: Follow the arc to Arcturus, and speed on (or drive a spike) to Spica.

Look for the Big Dipper

First, look for the Big Dipper in the northern sky. It’s highest in the evening sky in the northern spring and summer. Notice that the Big Dipper has a bowl and a long, curved handle. Follow the arc of the Dipper’s handle outward, away from the Dipper’s bowl. The first bright star you come to is orange Arcturus. Then speed on (or drive a spike) along this curving path. And the next bright star you come to is Spica.

Spica shines at magnitude 1.04, making it the brightest light in Virgo. In fact, it’s the 15th-brightest star visible from anywhere on Earth. It’s virtually the same brightness as Antares in the constellation Scorpius, so sometimes Antares is listed as the 15th and Spica as the 16th brightest.

Kite shaped constellation with a tail pointing to a dot labeled Arcturus and then to another dot labeled Spica.
In northern spring, look northeast to southeast in the evening. You’ll find the Big Dipper in the northeast evening sky. Then, follow the arc to Arcturus, and speed on to Spica.
Star chart showing Big Dipper with line to Arcturus continuing to Spica.
In northern summer, look northwest to southwest. You’ll find the Big Dipper in the northwest evening sky. But you can still follow the arc to Arcturus, and drive a speed on to Spica.

History and mythology of Spica

The name Spica is from the Latin word for “ear” (of grain). The general connotation is that Spica refers to an “ear of wheat.” Indeed, the star and the constellation Virgo itself were sometimes associated with the Greek goddess of the harvest, Demeter.

There are many names and stories for Spica’s constellation – Virgo – in mythology, and by association with Spica as well. Fewer stories refer to Spica independently. Many classical references refer to Virgo’s stars as a goddess or with some association with wheat or the harvest, since the sun passes through Virgo in the fall. In Greece and Rome she typically was Astraea, the very personification of Justice; or Persephone, daughter of Demeter. In Egypt, Virgo was identified with Isis, and Spica was considered her lute bearer. In ancient China, Spica was a special star of spring known as the Horn.

One Arabic name was Azimech, derived from words meaning Defenseless One or Solitary One. This title may be in reference to Spica’s solitary status with no other bright stars nearby. But Spica is not the most solitary star. That honor goes to Fomalhaut, sometimes called the Autumn Star.

Antique colored etching of winged young woman in long dress holding a wheat ear, with labeled scattered stars.
Here’s a classical illustration of the constellation Virgo the Maiden, with Spica embedded in the wheat in her left hand. Image via Urania’s Mirror/ Wikipedia (public domain).

How to see Spica from the Southern Hemisphere

Via Daniel Gaussen, Founder & Guide – Stargaze Mackenzie – New Zealand

For Southern Hemisphere observers, Spica’s constellation Virgo is one of the most prominent constellations of the autumn evening sky during May and June. Instead of looking south as Northern Hemisphere observers do, Southern Hemisphere stargazers should look toward the northern sky, where Virgo crosses the meridian high above the horizon.

The constellation appears upside down compared with Northern Hemisphere star charts, a reminder that our view of the celestial sphere is reversed. Despite this different orientation, the bright blue-white star Spica remains easy to identify as Virgo’s brightest star.

One of the easiest ways to find Spica is by using the so-called Spring Triangle, formed by Spica, Arcturus, and Regulus. This was named for Northern Hemisphere spring, so it’s actually seen during autumn in the south. During May and June evenings, these three bright stars dominate the northern sky, with Spica reaching highest of the three.

For observers in New Zealand’s South Island (around 45 latitude south), Spica reaches an altitude of about 61° when crossing the meridian, while from Auckland (37 latitude south) it culminates around 53° above the northern horizon.

Look for the distinctive shape of Virgo extending below Spica. The constellation forms a large, somewhat rectangular pattern of stars, although these stars are much fainter than Virgo’s brightest star.

Bottom line: Spica is the brightest star in Virgo. Spica is at least two stars orbiting extremely close together, distorting each other into egg shapes.

Virgo the Maiden represents a harvest goddess

The post Spica, the bright beacon of Virgo, is 2 stars first appeared on EarthSky.



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Blue Moon – and smallest moon of 2026 – on May 30-31


EarthSky’s Deborah Byrd talks about the May 30-31 Blue Moon and micromoon on this week’s livestream. Join the live dicusssion at noon CDT (17 UTC) on Wednesday, May 27. You can watch in the player above or on Youtube.

May 2026 has 2 full moons. The 1st was the full Flower Moon on May 1. The 2nd will be on overnight May 30-31. It’s a Blue Moon and a micromoon – or distant full moon – the most distant full moon of 2026.

The full Blue Moon overnight on May 30-31, 2026

The coming Blue Moon – at 8:45 UTC on May 31, 2026 – is a Blue Moon and the most distant full micromoon of this year. Blue Moons aren’t blue. But micromoons – near their monthly apogees, or most distant points from Earth for the month – are small moons on our sky’s dome (although not noticeably small to the human eye).

And this May 30-31 moon is 2026’s smallest moon. It’s about 252,360 miles (406,134 km) away, in contrast to an average moon distance of about 238,900 miles (384,472 km).

And so the May 30-31 full moon will be about 7% dimmer than an average full moon, and about 25–30% dimmer than a supermoon, or particularly close full moon.

The crest of this 2nd full moon of May falls at 8:45 UTC on May 31. That’s 3:45 a.m. CDT. So, if you live in the Americas, Europe or Africa, the moon is fullest for you during the night of May 30. But those west of the International Date Line (Australia, New Zealand and Asia) will find their fullest moon on the night of May 31.

The May 30-31 Blue Moon and micromoon will be near a bright star. It’s Antares, Heart of the Scorpion in the constellation Scorpius.

Don’t miss the next unmissable night sky event. Sign up for our free newsletter for daily night sky updates, as well as the latest science news.

Sky chart: A round full moon next to a red star close to the horizon on the slanted green ecliptic line.
On May 30, the full Blue Moon will appear close to the bright red star Antares, Heart of Scorpius the Scorpion. The crest of the full moon falls at 8:45 UTC on May 31. That’s 3:45 a.m. CDT. So, it’s almost as full when it rises in the east after sunset on May 30 and May 31. And it’s the 2nd and most distant of 3 full micromoons – or most distant full moons – in a row in 2026. So it’ll be the smallest full moon of 2026. Chart via EarthSky.

What’s a Blue Moon?

So, why is the May 30-31 full moon a Blue Moon? It won’t be blue in color.

Blue-colored moons in images – such as the images on this page – are often made using special blue camera filters or in a post-processing program such as PhotoShop. Usually, but not always.

True blue-colored moons are rare, and they aren’t necessarily full. They happen when Earth’s atmosphere contains dust or smoke particles of a certain size. The particles must be slightly wider than 900 nanometers.

So you might find particles of this size in the air above you when, for example, a wildfire is raging nearby. That’s because particles of this size are very efficient at scattering red light. When these particles are present in our air, and moonlight shines through them, the moon might appear blue in color.

People reported genuinely blue-looking moons after:

  • The eruption of Krakatoa in 1883.
  • The Mount St. Helens eruption in 1980.

To read more about truly blue-colored moons, click here

A full round blue-colored moon. A blue sphere with dark blotches.
A hypothetical representation of a blue-colored moon. Blue-colored moons are extremely rare. They happen in a region that has experienced a major wildfire or a volcanic eruption. For example, people saw blue-colored moons after Krakatoa’s 1883 eruption and Mount St. Helens’ 1980 eruption. Will the May 30-31, 2026, full Blue Moon look this color? No. It’ll be a Blue Moon in name only. Image via BlueHypercane761/ Wikimedia Commons.

What’s a monthly Blue Moon?

In modern times, most of us know that Blue Moons emerged from folklore. We call a full moon a Blue Moon when it’s the 2nd full moon of a single calendar month. This sort of Blue Moon happens seven times in every 19 years, or about every two to three years.

Let’s take a look at the eight calendar-month Blue-Moons (dates in UTC) in the present 19-year Metonic cycle:

  1. March 31, 2018
  2. October 31, 2020
  3. August 31, 2023
  4. May 31, 2026
  5. December 31, 2028
  6. September 30, 2031
  7. July 31, 2034
  8. January 31, 2037

Also, in a year where February has no full moon at all, as in the year 2018, you can have two full moons in January and two full moons in March. Thus, during those years there are two Blue Moons in single year. The next time we have two Blue Moons in one year is 2037.

How often do monthly Blue Moons happen? Often!

Crescent moon colored blue with blurred blue streaks of clouds.
Most Blue Moons are not blue in color. This photo of a moon among fast-moving clouds was created using special blue filters. Image via EarthSky friend Jv Noriega.

What’s a seasonal Blue Moon?

By season, we’re referring to the period of time between a solstice and an equinox, or vice versa. We’re talking about winter, spring, summer, fall. Each season typically lasts three months and typically has three full moons.

The next seasonal Blue Moon will fall on May 20, 2027. It happens because June 2027’s full moon falls about two days before the June solstice, early in the season of northern summer (southern winter). And thus, there’s enough time to squeeze four full moons into the 2027 March equinox season, which will end at the June solstice on June 21, 2027.

Weirdly, it’s not the 4th of these four full moons that’ll be called a Blue Moon. It’s the 3rd. Go figure.

Full moons (based on UTC date and time) between March 2027 equinox and June 2027 solstice:

March equinox: March 20, 2027

March full moon: March 22, 2027
April full moon: April 20, 2027
May full moon: May 20, 2027
June full moon: June 18, 2027

June solstice: June 21, 2027

Full moon, pale blue with darker blue blotches, in black space.
A full “blue” moon. This image was likely made using a blue filter. Photo via Eileen Rollin/ Unsplash.

How often do seasonal Blue Moons occur?

The phases of the moon recur on or near the same calendar dates every 19 years. That’s because 235 lunar months (235 returns to full moon) almost exactly equal 19 calendar years. Sure enough, 19 years from 2024 – in the year 2043 – the full moons will fall on June 22, July 21, August 20, and September 18.

Seasonal Blue Moons occur because there are 235 full moons but only 76 seasons (4 x 19 = 76) in this 19-year lunar cycle. If you have only three full moons in each season, then that’s a total of 228 full moons (76 x 3 = 228). Yet, there are 235 full moons in this 19-year cycle. So, these seven additional full moons (235 – 228 = 7) have to showcase seven four-full-moon seasons in this 19-year period. We list upcoming seasonal Blue Moon UTC dates – following the August 19, 2024, seasonal Blue Moon – below:

May 20, 2027
August 24, 2029
August 21, 2032
May 22, 2035
May 18, 2038
August 22, 2040
August 20, 2043

How often do seasonal Blue Moons happen? Like monthly Blue Moons, they happen a lot.

A seasonal and a monthly Blue Moon in a single year?

Very rarely, a seasonal Blue Moon (3rd of four full moons in one season) and a monthly Blue Moon (2nd of two full moons in one calendar month) can occur in the same calendar year. For this to happen, you need 13 full moons between successive December solstices for a seasonal Blue Moon and, generally, 13 full moons in one calendar year for a monthly Blue Moon.

This will next happen in the year 2048, when a monthly Blue Moon falls on January 31, and a seasonal Blue Moon on August 23.

Then 19 years later, in the year 2067, there will be a monthly Blue Moon on March 30, and a seasonal Blue Moon on November 20. In this instance, there are 13 full moons between successive December solstices, but only 12 full moons in one calendar year and no February 2067 full moon.

Why call them Blue Moons?

The idea of a Blue Moon as the 2nd full moon in a month is more recent – more modern – than the idea of a Blue Moon as the 3rd of four full moons in a season. It stemmed from the March 1946 issue of Sky and Telescope magazine. The magazine published an article called “Once in a Blue Moon” by James Hugh Pruett. Pruett was referring to the 1937 Maine Farmer’s Almanac, which defined Blue Moons as the 3rd of four full moons in a season. But he inadvertently simplified the definition. He wrote:

Seven times in 19 years there were – and still are – 13 full moons in a year. This gives 11 months with one full moon each and one with two. This second in a month, so I interpret it, was called Blue Moon.

Had James Hugh Pruett looked at the actual date of the 1937 Blue Moon, he would have found that it had occurred August 21, 1937. Also, there were only 12 full moons in 1937. You generally need 13 full moons in one calendar year to have two full moons in one calendar month.

However, that fortuitous oversight gave birth to a new and perfectly understandable definition for Blue Moon.

Closeup of moon showing craters and dark areas, all in indigo colors.
It’s very rare that you would see a moon that’s actually blue in color. This photo was created using special filters. Most Blue Moons you hear about are Blue in name only. Image via our friend Jv Noriega.

Blue Moons as modern folklore

The notion of a Blue Moon as the 2nd full moon of a calendar month was buried for decades. Then, in the late 1970s, EarthSky’s Deborah Byrd happened upon a copy of the old 1946 issue of Sky and Telescope in the stacks of the Peridier Library at the University of Texas Astronomy Department. Afterward, she began using the term Blue Moon to describe the second full moon in a calendar month on the radio series StarDate, which she wrote and produced.

Later, this definition of Blue Moon was also popularized by a book for children by Margot McLoone-Basta, called The Kids’ World Almanac of Records and Facts, published in New York by World Almanac Publications in 1985. The second-full-moon-in-a-month definition was also used in the board game Trivial Pursuit.

Today, it has become part of modern folklore. As the folklorist Philip Hiscock wrote in his comprehensive article Once in a Blue Moon:

‘Old folklore’ it is not, but real folklore it is.

Bottom line: The full moon overnight on May 30-31, 2026, is a Blue Moon. What is a Blue Moon? The 2nd of two full moons in a calendar month? Or the 3rd of four full moons in a single season? The answer is … both!

Phases of the moon: 2001 to 2100

Solstices and equinoxes: 2001 to 2100

Possible to have only 2 full moons in a single season?

The post Blue Moon – and smallest moon of 2026 – on May 30-31 first appeared on EarthSky.



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EarthSky’s Deborah Byrd talks about the May 30-31 Blue Moon and micromoon on this week’s livestream. Join the live dicusssion at noon CDT (17 UTC) on Wednesday, May 27. You can watch in the player above or on Youtube.

May 2026 has 2 full moons. The 1st was the full Flower Moon on May 1. The 2nd will be on overnight May 30-31. It’s a Blue Moon and a micromoon – or distant full moon – the most distant full moon of 2026.

The full Blue Moon overnight on May 30-31, 2026

The coming Blue Moon – at 8:45 UTC on May 31, 2026 – is a Blue Moon and the most distant full micromoon of this year. Blue Moons aren’t blue. But micromoons – near their monthly apogees, or most distant points from Earth for the month – are small moons on our sky’s dome (although not noticeably small to the human eye).

And this May 30-31 moon is 2026’s smallest moon. It’s about 252,360 miles (406,134 km) away, in contrast to an average moon distance of about 238,900 miles (384,472 km).

And so the May 30-31 full moon will be about 7% dimmer than an average full moon, and about 25–30% dimmer than a supermoon, or particularly close full moon.

The crest of this 2nd full moon of May falls at 8:45 UTC on May 31. That’s 3:45 a.m. CDT. So, if you live in the Americas, Europe or Africa, the moon is fullest for you during the night of May 30. But those west of the International Date Line (Australia, New Zealand and Asia) will find their fullest moon on the night of May 31.

The May 30-31 Blue Moon and micromoon will be near a bright star. It’s Antares, Heart of the Scorpion in the constellation Scorpius.

Don’t miss the next unmissable night sky event. Sign up for our free newsletter for daily night sky updates, as well as the latest science news.

Sky chart: A round full moon next to a red star close to the horizon on the slanted green ecliptic line.
On May 30, the full Blue Moon will appear close to the bright red star Antares, Heart of Scorpius the Scorpion. The crest of the full moon falls at 8:45 UTC on May 31. That’s 3:45 a.m. CDT. So, it’s almost as full when it rises in the east after sunset on May 30 and May 31. And it’s the 2nd and most distant of 3 full micromoons – or most distant full moons – in a row in 2026. So it’ll be the smallest full moon of 2026. Chart via EarthSky.

What’s a Blue Moon?

So, why is the May 30-31 full moon a Blue Moon? It won’t be blue in color.

Blue-colored moons in images – such as the images on this page – are often made using special blue camera filters or in a post-processing program such as PhotoShop. Usually, but not always.

True blue-colored moons are rare, and they aren’t necessarily full. They happen when Earth’s atmosphere contains dust or smoke particles of a certain size. The particles must be slightly wider than 900 nanometers.

So you might find particles of this size in the air above you when, for example, a wildfire is raging nearby. That’s because particles of this size are very efficient at scattering red light. When these particles are present in our air, and moonlight shines through them, the moon might appear blue in color.

People reported genuinely blue-looking moons after:

  • The eruption of Krakatoa in 1883.
  • The Mount St. Helens eruption in 1980.

To read more about truly blue-colored moons, click here

A full round blue-colored moon. A blue sphere with dark blotches.
A hypothetical representation of a blue-colored moon. Blue-colored moons are extremely rare. They happen in a region that has experienced a major wildfire or a volcanic eruption. For example, people saw blue-colored moons after Krakatoa’s 1883 eruption and Mount St. Helens’ 1980 eruption. Will the May 30-31, 2026, full Blue Moon look this color? No. It’ll be a Blue Moon in name only. Image via BlueHypercane761/ Wikimedia Commons.

What’s a monthly Blue Moon?

In modern times, most of us know that Blue Moons emerged from folklore. We call a full moon a Blue Moon when it’s the 2nd full moon of a single calendar month. This sort of Blue Moon happens seven times in every 19 years, or about every two to three years.

Let’s take a look at the eight calendar-month Blue-Moons (dates in UTC) in the present 19-year Metonic cycle:

  1. March 31, 2018
  2. October 31, 2020
  3. August 31, 2023
  4. May 31, 2026
  5. December 31, 2028
  6. September 30, 2031
  7. July 31, 2034
  8. January 31, 2037

Also, in a year where February has no full moon at all, as in the year 2018, you can have two full moons in January and two full moons in March. Thus, during those years there are two Blue Moons in single year. The next time we have two Blue Moons in one year is 2037.

How often do monthly Blue Moons happen? Often!

Crescent moon colored blue with blurred blue streaks of clouds.
Most Blue Moons are not blue in color. This photo of a moon among fast-moving clouds was created using special blue filters. Image via EarthSky friend Jv Noriega.

What’s a seasonal Blue Moon?

By season, we’re referring to the period of time between a solstice and an equinox, or vice versa. We’re talking about winter, spring, summer, fall. Each season typically lasts three months and typically has three full moons.

The next seasonal Blue Moon will fall on May 20, 2027. It happens because June 2027’s full moon falls about two days before the June solstice, early in the season of northern summer (southern winter). And thus, there’s enough time to squeeze four full moons into the 2027 March equinox season, which will end at the June solstice on June 21, 2027.

Weirdly, it’s not the 4th of these four full moons that’ll be called a Blue Moon. It’s the 3rd. Go figure.

Full moons (based on UTC date and time) between March 2027 equinox and June 2027 solstice:

March equinox: March 20, 2027

March full moon: March 22, 2027
April full moon: April 20, 2027
May full moon: May 20, 2027
June full moon: June 18, 2027

June solstice: June 21, 2027

Full moon, pale blue with darker blue blotches, in black space.
A full “blue” moon. This image was likely made using a blue filter. Photo via Eileen Rollin/ Unsplash.

How often do seasonal Blue Moons occur?

The phases of the moon recur on or near the same calendar dates every 19 years. That’s because 235 lunar months (235 returns to full moon) almost exactly equal 19 calendar years. Sure enough, 19 years from 2024 – in the year 2043 – the full moons will fall on June 22, July 21, August 20, and September 18.

Seasonal Blue Moons occur because there are 235 full moons but only 76 seasons (4 x 19 = 76) in this 19-year lunar cycle. If you have only three full moons in each season, then that’s a total of 228 full moons (76 x 3 = 228). Yet, there are 235 full moons in this 19-year cycle. So, these seven additional full moons (235 – 228 = 7) have to showcase seven four-full-moon seasons in this 19-year period. We list upcoming seasonal Blue Moon UTC dates – following the August 19, 2024, seasonal Blue Moon – below:

May 20, 2027
August 24, 2029
August 21, 2032
May 22, 2035
May 18, 2038
August 22, 2040
August 20, 2043

How often do seasonal Blue Moons happen? Like monthly Blue Moons, they happen a lot.

A seasonal and a monthly Blue Moon in a single year?

Very rarely, a seasonal Blue Moon (3rd of four full moons in one season) and a monthly Blue Moon (2nd of two full moons in one calendar month) can occur in the same calendar year. For this to happen, you need 13 full moons between successive December solstices for a seasonal Blue Moon and, generally, 13 full moons in one calendar year for a monthly Blue Moon.

This will next happen in the year 2048, when a monthly Blue Moon falls on January 31, and a seasonal Blue Moon on August 23.

Then 19 years later, in the year 2067, there will be a monthly Blue Moon on March 30, and a seasonal Blue Moon on November 20. In this instance, there are 13 full moons between successive December solstices, but only 12 full moons in one calendar year and no February 2067 full moon.

Why call them Blue Moons?

The idea of a Blue Moon as the 2nd full moon in a month is more recent – more modern – than the idea of a Blue Moon as the 3rd of four full moons in a season. It stemmed from the March 1946 issue of Sky and Telescope magazine. The magazine published an article called “Once in a Blue Moon” by James Hugh Pruett. Pruett was referring to the 1937 Maine Farmer’s Almanac, which defined Blue Moons as the 3rd of four full moons in a season. But he inadvertently simplified the definition. He wrote:

Seven times in 19 years there were – and still are – 13 full moons in a year. This gives 11 months with one full moon each and one with two. This second in a month, so I interpret it, was called Blue Moon.

Had James Hugh Pruett looked at the actual date of the 1937 Blue Moon, he would have found that it had occurred August 21, 1937. Also, there were only 12 full moons in 1937. You generally need 13 full moons in one calendar year to have two full moons in one calendar month.

However, that fortuitous oversight gave birth to a new and perfectly understandable definition for Blue Moon.

Closeup of moon showing craters and dark areas, all in indigo colors.
It’s very rare that you would see a moon that’s actually blue in color. This photo was created using special filters. Most Blue Moons you hear about are Blue in name only. Image via our friend Jv Noriega.

Blue Moons as modern folklore

The notion of a Blue Moon as the 2nd full moon of a calendar month was buried for decades. Then, in the late 1970s, EarthSky’s Deborah Byrd happened upon a copy of the old 1946 issue of Sky and Telescope in the stacks of the Peridier Library at the University of Texas Astronomy Department. Afterward, she began using the term Blue Moon to describe the second full moon in a calendar month on the radio series StarDate, which she wrote and produced.

Later, this definition of Blue Moon was also popularized by a book for children by Margot McLoone-Basta, called The Kids’ World Almanac of Records and Facts, published in New York by World Almanac Publications in 1985. The second-full-moon-in-a-month definition was also used in the board game Trivial Pursuit.

Today, it has become part of modern folklore. As the folklorist Philip Hiscock wrote in his comprehensive article Once in a Blue Moon:

‘Old folklore’ it is not, but real folklore it is.

Bottom line: The full moon overnight on May 30-31, 2026, is a Blue Moon. What is a Blue Moon? The 2nd of two full moons in a calendar month? Or the 3rd of four full moons in a single season? The answer is … both!

Phases of the moon: 2001 to 2100

Solstices and equinoxes: 2001 to 2100

Possible to have only 2 full moons in a single season?

The post Blue Moon – and smallest moon of 2026 – on May 30-31 first appeared on EarthSky.



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Hot Jupiter exoplanet has cloudy mornings and clear evenings

Large banded planet with huge pole to pole band of white fluffy clouds at edge of nightside.
Artist’s concept of WASP-94A b, a hot Jupiter-type exoplanet about 700 light-years away. New observations by the James Webb Space Telescope show that sandy clouds fill the skies in the morning, but dissipate by the evening. Image via Hannah Robbins/ Johns Hopkins University/ EurekAlert! (CC BY).
  • WASP-94A b is a hot Jupiter exoplanet about 700 light-years from Earth. Astronomers recently performed more observations of it with the James Webb Space Telescope.
  • The planet has cloudy morning and clear evenings, Webb found. Clouds of sandy particles form in the mornings and the dissipate by the evening.
  • The cloud-free evenings also allowed Webb to analyze the atmosphere itself more clearly, without clouds contaminating the data.

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

Cloudy mornings on a hot Jupiter exoplanet

On a hot Jupiter-type exoplanet about 700 light-years away, sand clouds build up every morning, but then dissipate by nightfall. That’s the amazingly precise finding of a team of researchers at Johns Hopkins University, announced on May 21, 2026.

The planet – WASP-94A b – is tidally locked to its star. So it always keeps a single side facing its star, which is a little hotter, larger, and more luminous than our sun. No one has directly measured the rotation period of WASP-94A b. But its orbital period is about four Earth days. So it probably rotates once in that amount of time (much as our moon takes about a month to orbit Earth, while rotating once on its axis).

The clouds appear to form on the cooler nightside of WASP-94A b. They circulate toward this world’s dayside and ultimately evaporate in the intense heat. Why so intense? Because WASP-94A b is orbiting super-closely to its star, only about 5 million miles (8 million km) away. That’s in contrast to Earth at 93 million miles (150 million km), or the sun’s innermost planet, Mercury, which gets no closer than 29 million miles (47 million km) to our star.

And, by isolating the clouds in their analysis, the researchers said they could better determine the composition of the planet’s atmosphere.

This is one of just a handful of times that astronomers have detected cloud cycles on a hot Jupiter. The researchers made the observations with the James Webb Space Telescope.

They published the new peer-reviewed findings in the journal Science on May 21, 2026. There is also an earlier preprint version of the paper from last year available.

Observing the transit of WASP-94A b

The Webb telescope observed the planet as it transited – passed in front of – its star. The researchers took measurements as the planet started to transit, and as it finished the transit. At the leading edge, the atmosphere flows from the nightside to the dayside. This makes it the morning. But at the trailing edge, the atmosphere flows from the dayside to the nightside, making it evening.

The observations revealed that the morning atmosphere is filled with clouds made of magnesium silicate – aka talc – a common mineral found in rocks on Earth. The evening atmosphere, though, is clear and cloud-free.

Cloudy Mornings And Clear Evenings On Giant Extrasolar World WASP-94A bastrobiology.com/2025/05/clou… #astrobiology #exoplanet #atmosphere

Astrobiology (@astrobiology.bsky.social) 2025-05-19T17:22:22.927Z

Now on @sciam.bsky.social: NASA's JWST just delivered a fascinating weather report for the distant exoplanet WASP-94A b, finding the gas-giant world has partly cloudy skies. By @krcallaway.bsky.social.https://ift.tt/Dc9PvoV…

Lee Billings (@leebillings.bsky.social) 2026-05-21T18:21:32.933Z

What is causing this?

So, what is the reason for this interesting atmospheric phenomenon? Right now, the researchers have two main hypotheses:

First, powerful winds could be lifting clouds higher up on the cooler nightside of the planet. Then, the clouds plunge back down on the hotter dayside. This buries the clouds much deeper in the atmosphere where they remain hidden.

Or, another possibility is that this process is similar to when fog burns off on Earth. The clouds form on the cooler nightside of the planet. Then, they drift into the hotter dayside. Because it is so hot, the chemicals in the clouds boil away and the clouds vaporize.

As co-author and program principal investigator David Sing at Johns Hopkins University said:

It was a huge surprise. People have expected some differences, like it’s cooler in the morning than the evening; that’s something natural that we experience here on Earth. But what we saw was a real dichotomy between the weather on both sides of the planet, and huge differences in cloud coverage, and that changes our whole picture of the planet.

Smiling young man with short black hair wearing eyeglasses and a red sweater.
Sagnick Mukherjee at Arizona State University is the lead author of the new study about clouds on WASP-94A b. Image via GitHub.

Cloud-free evenings

The evenings being free of clouds gave the researchers an opportunity. They could study the atmosphere itself more clearly with Webb. The Hubble Space Telescope isn’t able to do this. Lead author Sagnick Mukherjee at Arizona State University explained:

With the Hubble telescope, when we used to do this type of observation, we got an average view of the whole planet with data from the clouds and the atmosphere squished together and indistinguishable. This approach with the JWST lets us localize our observations, which helped us see the cloud cycle.

And what did the observations show? That WASP-94A b is actually more like Jupiter than first thought. Earlier observations suggested that WASP-94A b had hundreds of times more oxygen and carbon than Jupiter. But now the newer, cleaner analysis shows that really only has five times more. That fits much better into current planetary formation models.

Large planet with multicolored swirly bands. There is a big orange spot on its surface.
View larger. | Jupiter as captured by the Juno spacecraft in February 2019. The new study also shows that WASP-94A b is more like Jupiter than previously thought, with only 5 times more oxygen and carbon. Image via NASA/ JPL-Caltech/ SwRI/ MSSS/ Kevin M. Gill.

A clearer view of the atmosphere

The new observations are a big step in being able to study both clouds and the atmosphere on exoplanets. Sing said:

I’ve been looking at exoplanets for 20 years, and general cloudiness has been a thorn in our side. We’ve known for quite a while that clouds are pervasive on hot Jupiter planets, which is annoying because it’s like trying to look at the planet through a foggy window. Not only have we been able to clear the view, but we can finally pin down what the clouds are made out of and how they’re condensing and evaporating as they move around the planet.

Bottom line: New observations with the Webb space telescope of the hot Jupiter exoplanet WASP-94A b show that sandy clouds fill the morning skies, but dissipate by evening.

Source: Cloudy mornings and clear evenings on a gas giant exoplanet

Source (preprint): Cloudy mornings and clear evenings on a giant extrasolar world

Via Johns Hopkins University

Read more: Double hot Jupiters: How do these rare gigantic worlds form?

Read more: A hot Jupiter exoplanet’s dark side revealed

The post Hot Jupiter exoplanet has cloudy mornings and clear evenings first appeared on EarthSky.



from EarthSky https://ift.tt/SMxV5gd
Large banded planet with huge pole to pole band of white fluffy clouds at edge of nightside.
Artist’s concept of WASP-94A b, a hot Jupiter-type exoplanet about 700 light-years away. New observations by the James Webb Space Telescope show that sandy clouds fill the skies in the morning, but dissipate by the evening. Image via Hannah Robbins/ Johns Hopkins University/ EurekAlert! (CC BY).
  • WASP-94A b is a hot Jupiter exoplanet about 700 light-years from Earth. Astronomers recently performed more observations of it with the James Webb Space Telescope.
  • The planet has cloudy morning and clear evenings, Webb found. Clouds of sandy particles form in the mornings and the dissipate by the evening.
  • The cloud-free evenings also allowed Webb to analyze the atmosphere itself more clearly, without clouds contaminating the data.

You deserve a daily dose of good news. For the latest in science and the night sky, click here to subscribe to our free daily newsletter.

Cloudy mornings on a hot Jupiter exoplanet

On a hot Jupiter-type exoplanet about 700 light-years away, sand clouds build up every morning, but then dissipate by nightfall. That’s the amazingly precise finding of a team of researchers at Johns Hopkins University, announced on May 21, 2026.

The planet – WASP-94A b – is tidally locked to its star. So it always keeps a single side facing its star, which is a little hotter, larger, and more luminous than our sun. No one has directly measured the rotation period of WASP-94A b. But its orbital period is about four Earth days. So it probably rotates once in that amount of time (much as our moon takes about a month to orbit Earth, while rotating once on its axis).

The clouds appear to form on the cooler nightside of WASP-94A b. They circulate toward this world’s dayside and ultimately evaporate in the intense heat. Why so intense? Because WASP-94A b is orbiting super-closely to its star, only about 5 million miles (8 million km) away. That’s in contrast to Earth at 93 million miles (150 million km), or the sun’s innermost planet, Mercury, which gets no closer than 29 million miles (47 million km) to our star.

And, by isolating the clouds in their analysis, the researchers said they could better determine the composition of the planet’s atmosphere.

This is one of just a handful of times that astronomers have detected cloud cycles on a hot Jupiter. The researchers made the observations with the James Webb Space Telescope.

They published the new peer-reviewed findings in the journal Science on May 21, 2026. There is also an earlier preprint version of the paper from last year available.

Observing the transit of WASP-94A b

The Webb telescope observed the planet as it transited – passed in front of – its star. The researchers took measurements as the planet started to transit, and as it finished the transit. At the leading edge, the atmosphere flows from the nightside to the dayside. This makes it the morning. But at the trailing edge, the atmosphere flows from the dayside to the nightside, making it evening.

The observations revealed that the morning atmosphere is filled with clouds made of magnesium silicate – aka talc – a common mineral found in rocks on Earth. The evening atmosphere, though, is clear and cloud-free.

Cloudy Mornings And Clear Evenings On Giant Extrasolar World WASP-94A bastrobiology.com/2025/05/clou… #astrobiology #exoplanet #atmosphere

Astrobiology (@astrobiology.bsky.social) 2025-05-19T17:22:22.927Z

Now on @sciam.bsky.social: NASA's JWST just delivered a fascinating weather report for the distant exoplanet WASP-94A b, finding the gas-giant world has partly cloudy skies. By @krcallaway.bsky.social.https://ift.tt/Dc9PvoV…

Lee Billings (@leebillings.bsky.social) 2026-05-21T18:21:32.933Z

What is causing this?

So, what is the reason for this interesting atmospheric phenomenon? Right now, the researchers have two main hypotheses:

First, powerful winds could be lifting clouds higher up on the cooler nightside of the planet. Then, the clouds plunge back down on the hotter dayside. This buries the clouds much deeper in the atmosphere where they remain hidden.

Or, another possibility is that this process is similar to when fog burns off on Earth. The clouds form on the cooler nightside of the planet. Then, they drift into the hotter dayside. Because it is so hot, the chemicals in the clouds boil away and the clouds vaporize.

As co-author and program principal investigator David Sing at Johns Hopkins University said:

It was a huge surprise. People have expected some differences, like it’s cooler in the morning than the evening; that’s something natural that we experience here on Earth. But what we saw was a real dichotomy between the weather on both sides of the planet, and huge differences in cloud coverage, and that changes our whole picture of the planet.

Smiling young man with short black hair wearing eyeglasses and a red sweater.
Sagnick Mukherjee at Arizona State University is the lead author of the new study about clouds on WASP-94A b. Image via GitHub.

Cloud-free evenings

The evenings being free of clouds gave the researchers an opportunity. They could study the atmosphere itself more clearly with Webb. The Hubble Space Telescope isn’t able to do this. Lead author Sagnick Mukherjee at Arizona State University explained:

With the Hubble telescope, when we used to do this type of observation, we got an average view of the whole planet with data from the clouds and the atmosphere squished together and indistinguishable. This approach with the JWST lets us localize our observations, which helped us see the cloud cycle.

And what did the observations show? That WASP-94A b is actually more like Jupiter than first thought. Earlier observations suggested that WASP-94A b had hundreds of times more oxygen and carbon than Jupiter. But now the newer, cleaner analysis shows that really only has five times more. That fits much better into current planetary formation models.

Large planet with multicolored swirly bands. There is a big orange spot on its surface.
View larger. | Jupiter as captured by the Juno spacecraft in February 2019. The new study also shows that WASP-94A b is more like Jupiter than previously thought, with only 5 times more oxygen and carbon. Image via NASA/ JPL-Caltech/ SwRI/ MSSS/ Kevin M. Gill.

A clearer view of the atmosphere

The new observations are a big step in being able to study both clouds and the atmosphere on exoplanets. Sing said:

I’ve been looking at exoplanets for 20 years, and general cloudiness has been a thorn in our side. We’ve known for quite a while that clouds are pervasive on hot Jupiter planets, which is annoying because it’s like trying to look at the planet through a foggy window. Not only have we been able to clear the view, but we can finally pin down what the clouds are made out of and how they’re condensing and evaporating as they move around the planet.

Bottom line: New observations with the Webb space telescope of the hot Jupiter exoplanet WASP-94A b show that sandy clouds fill the morning skies, but dissipate by evening.

Source: Cloudy mornings and clear evenings on a gas giant exoplanet

Source (preprint): Cloudy mornings and clear evenings on a giant extrasolar world

Via Johns Hopkins University

Read more: Double hot Jupiters: How do these rare gigantic worlds form?

Read more: A hot Jupiter exoplanet’s dark side revealed

The post Hot Jupiter exoplanet has cloudy mornings and clear evenings first appeared on EarthSky.



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Meet Crux, the constellation of the Southern Cross

Star chart: 4 labeled stars at ends of cross arms and small dots for a labeled star cluster.
Crux is the constellation of the Southern Cross. And it lies deep in Southern Hemisphere skies. Image via EarthSky.

Your support = more stars, more science, more wonder. Donate to EarthSky and be part of something bigger.

If you’re in the Southern Hemisphere, Crux the Southern Cross is one of the easiest constellations you can identify. It’s also one of the most famous! And it’s a reliable marker to the south celestial pole, the point around which the entire southern sky turns.

Crux consists of four relatively bright stars, close to one another and suggestive of a cross. This constellation is circumpolar, staying above the horizon all year round for observers at and south of 34 degrees south latitude. So, for example:

  • At Sydney, Australia, (~34° S), most or all of Crux is circumpolar.
  • At Buenos Aires, Argentina, (~35° S), it’s comfortably circumpolar.
  • At Cape Town, South Africa, (~34° S), same story.
  • Farther north – say at the equator – Crux rises and sets seasonally.
  • North of about 27 degrees north latitude, Crux never rises at all.

In many ways, Crux is almost the mirror opposite of northern circumpolar constellations like Ursa Major the Greater Bear, with its famous Big Dipper asterism. Like the Big Dipper for northern observers, the Southern Cross is the southern sky’s iconic “always there” pattern.

And for a short time each year it can be seen by those in the southern reaches of the Northern Hemisphere. Jump to that section.

How to see it from the Southern Hemisphere

Crux lies between the constellations Centaurus the Centaur and Musca the Fly. You can locate it simply by looking for four bright stars close together. The stars are less than 5 degrees apart. Five degrees is about the width of your three middle fingers held at arm’s length.

The compact size of Crux makes it the smallest of all the 88 constellations.

And Crux does resemble a cross. But it could also be considered kite-shaped.

Want an exact view from your location? Try Stellarium

Star chart: Milky Way with stars forming a cross and neighboring constellations.
Crux the Southern Cross lies in front of the Milky Way with Centaurus and Musca nearby. Image via Stellarium. Used with permission.

How to see it from the Northern Hemisphere

Seeing the Southern Cross from the Northern Hemisphere is a matter of your location + timing + atmosphere + horizon quality.

First, your location. Know what your latitude allows. Crux sits around -60 degrees declination, so:

  • At the equator (0 degrees) it can rise to ~30° high. That’s easy to see if the sky is clear.
  • At 26 degrees north latitude it barely scrapes the sky at about 4 degrees above the southern horizon.
  • At ~27 degrees north latitude and northward it never rises above the horizon.

So at 26 degrees north latitude you are in the extreme edge zone. You can’t just look up and observe the Southern Cross. Instead, you must hunt for it at the most distorted layer of atmosphere above your southern horizon. And you must be hunting at the exact right time.

More Northern Hemisphere viewing tips

Consider the timing. May is a good time to find Crux in the evening sky from the Northern Hemisphere. It’s visible in other months, too, but not at such a convenient time. In March, you have to wait until about 1 a.m. your local time to catch the Southern Cross at its highest elevation. In December and January, you have to catch it before dawn.

No matter the hour or date, Crux climbs to its highest point – crosses your sky’s meridian – in the sky when it’s due south. It’s easy to visualize a cross within this pattern of stars, because the pattern stands upright over your southern horizon.

And speaking of your horizon … To see the Southern Cross from anywhere in the Northern Hemisphere, you’ll want a clear, unobstructed southern horizon. A dark sky will be best. Visit EarthSky’s Best Places to Stargaze.

Read more about seeing the Southern Cross from the Northern Hemisphere.

Want an exact view from your location? Try Stellarium

A man seen from behind looking outward over a city toward the Southern Cross with stars labeled.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, India, caught the Southern Cross at its highest point around midnight (its midnight culmination) on March 6, 2021. In April and May, the Southern Cross reaches its highest point in the sky earlier in the evening. Thank you, Prateek!

Stars of Crux

The brightest star of the Southern Cross is Alpha Crucis, or Acrux. It’s the bottom star of the Cross and shines at magnitude 0.77 from a distance of 320 light-years. It’s also the 12th brightest star in the sky.

Moving in a clockwise circle around the Cross we come to the 2nd brightest star, Beta Crucis, sometimes called Becrux or Mimosa. Beta Crucis is magnitude 1.25 from a distance of 350 light-years.

Next, on the top of the Cross, is Gamma Crucis, or Gacrux. Gacrux shines at magnitude 1.59 at a distance of 88 light-years. Finally, on the right side of the cross, is Delta Crucis. It shines at magnitude 2.79 from a distance of 360 light-years.

Star chart in white with black dots for stars showing cross shape at center.
The stars of Crux the Southern Cross. Image via/ IAU/ Sky and Telescope/ Wikimedia Commons.

Use the Southern Cross to find due south

Arrows coming from the Southern Cross and Archernar meet in the middle, where the South Celestial Pole is.
Method #1. The south celestial pole is located halfway between Gacrux, the head of the Southern Cross, and the bright star Achernar. For a practical trick, place one hand at the Cross and the other at Achernar. Now bring them together in a clap! Your hands should meet right at the south celestial pole. Chart via EarthSky.
Arrows from the Southern Cross and Alpha Centauri converge at the south celestial pole.
Method #2. Draw an imaginary line extending the long axis of the Southern Cross, and another one bisecting the 2 “Pointer Stars,” Alpha and Beta Centauri. The south celestial pole lies at the intersection between those 2 lines. Chart via EarthSky.
Arrow, divided into 4 segments each equal to the length of the Southern Cross, from the cross to the south celestial pole.
Method #3. To locate the south celestial pole, extend the long axis of the Southern Cross from the head of the cross through its foot, 4 times its own length. Chart via EarthSky.

The Jewel Box and other clusters in Crux

The Jewel Box is one of the most beautiful open clusters in the Southern Hemisphere. It lies just 1 degree from Beta Crucis. The Jewel Box, or NGC 4755, is bright at magnitude 4.2. Kappa Crucis, a magnitude 5.89 star, lies inside.

You can see the Jewel Box without optical aid. But a pair of binoculars or a telescope will bring more of the stars into focus.

Can you see color differences between these glittering gems?

Glittering cluster of mostly blue stars with one red one near center.
NGC 4755, or the Jewel Box, from ESO’s La Silla Observatory. Image via ESO.

The Coalsack Nebula

The easiest dark nebula to see in the sky is the Coalsack Nebula, found in the southeastern corner of Crux. The Coalsack is a dark, cloudy patch of dust and gas that obscures an entire swath of the Milky Way’s stars that lies behind it.

Large irregular black area surrounded by starfield and bright blue star at top.
Meet the Coalsack, a huge cloud of gas and dust in space. The dust in this and other dark nebulae absorb and scatter the light of background stars. This creates a region of the sky that looks starless, but it’s really a place where new stars are forming. May is one of the best months to see the Coalsack in the constellation Crux in the Southern Hemisphere. This image is from the Wide Field Imager on the MPG/ESO 2.2-meter telescope. Image via ESO.

Bottom line: Crux, the constellation of the Southern Cross, is a hallmark of southern skies and contains the open cluster known as the Jewel Box.

Read more: How to see the Southern Cross from the Northern Hemisphere

The post Meet Crux, the constellation of the Southern Cross first appeared on EarthSky.



from EarthSky https://ift.tt/XTkY6ey
Star chart: 4 labeled stars at ends of cross arms and small dots for a labeled star cluster.
Crux is the constellation of the Southern Cross. And it lies deep in Southern Hemisphere skies. Image via EarthSky.

Your support = more stars, more science, more wonder. Donate to EarthSky and be part of something bigger.

If you’re in the Southern Hemisphere, Crux the Southern Cross is one of the easiest constellations you can identify. It’s also one of the most famous! And it’s a reliable marker to the south celestial pole, the point around which the entire southern sky turns.

Crux consists of four relatively bright stars, close to one another and suggestive of a cross. This constellation is circumpolar, staying above the horizon all year round for observers at and south of 34 degrees south latitude. So, for example:

  • At Sydney, Australia, (~34° S), most or all of Crux is circumpolar.
  • At Buenos Aires, Argentina, (~35° S), it’s comfortably circumpolar.
  • At Cape Town, South Africa, (~34° S), same story.
  • Farther north – say at the equator – Crux rises and sets seasonally.
  • North of about 27 degrees north latitude, Crux never rises at all.

In many ways, Crux is almost the mirror opposite of northern circumpolar constellations like Ursa Major the Greater Bear, with its famous Big Dipper asterism. Like the Big Dipper for northern observers, the Southern Cross is the southern sky’s iconic “always there” pattern.

And for a short time each year it can be seen by those in the southern reaches of the Northern Hemisphere. Jump to that section.

How to see it from the Southern Hemisphere

Crux lies between the constellations Centaurus the Centaur and Musca the Fly. You can locate it simply by looking for four bright stars close together. The stars are less than 5 degrees apart. Five degrees is about the width of your three middle fingers held at arm’s length.

The compact size of Crux makes it the smallest of all the 88 constellations.

And Crux does resemble a cross. But it could also be considered kite-shaped.

Want an exact view from your location? Try Stellarium

Star chart: Milky Way with stars forming a cross and neighboring constellations.
Crux the Southern Cross lies in front of the Milky Way with Centaurus and Musca nearby. Image via Stellarium. Used with permission.

How to see it from the Northern Hemisphere

Seeing the Southern Cross from the Northern Hemisphere is a matter of your location + timing + atmosphere + horizon quality.

First, your location. Know what your latitude allows. Crux sits around -60 degrees declination, so:

  • At the equator (0 degrees) it can rise to ~30° high. That’s easy to see if the sky is clear.
  • At 26 degrees north latitude it barely scrapes the sky at about 4 degrees above the southern horizon.
  • At ~27 degrees north latitude and northward it never rises above the horizon.

So at 26 degrees north latitude you are in the extreme edge zone. You can’t just look up and observe the Southern Cross. Instead, you must hunt for it at the most distorted layer of atmosphere above your southern horizon. And you must be hunting at the exact right time.

More Northern Hemisphere viewing tips

Consider the timing. May is a good time to find Crux in the evening sky from the Northern Hemisphere. It’s visible in other months, too, but not at such a convenient time. In March, you have to wait until about 1 a.m. your local time to catch the Southern Cross at its highest elevation. In December and January, you have to catch it before dawn.

No matter the hour or date, Crux climbs to its highest point – crosses your sky’s meridian – in the sky when it’s due south. It’s easy to visualize a cross within this pattern of stars, because the pattern stands upright over your southern horizon.

And speaking of your horizon … To see the Southern Cross from anywhere in the Northern Hemisphere, you’ll want a clear, unobstructed southern horizon. A dark sky will be best. Visit EarthSky’s Best Places to Stargaze.

Read more about seeing the Southern Cross from the Northern Hemisphere.

Want an exact view from your location? Try Stellarium

A man seen from behind looking outward over a city toward the Southern Cross with stars labeled.
View at EarthSky Community Photos. | Prateek Pandey in Bhopal, India, caught the Southern Cross at its highest point around midnight (its midnight culmination) on March 6, 2021. In April and May, the Southern Cross reaches its highest point in the sky earlier in the evening. Thank you, Prateek!

Stars of Crux

The brightest star of the Southern Cross is Alpha Crucis, or Acrux. It’s the bottom star of the Cross and shines at magnitude 0.77 from a distance of 320 light-years. It’s also the 12th brightest star in the sky.

Moving in a clockwise circle around the Cross we come to the 2nd brightest star, Beta Crucis, sometimes called Becrux or Mimosa. Beta Crucis is magnitude 1.25 from a distance of 350 light-years.

Next, on the top of the Cross, is Gamma Crucis, or Gacrux. Gacrux shines at magnitude 1.59 at a distance of 88 light-years. Finally, on the right side of the cross, is Delta Crucis. It shines at magnitude 2.79 from a distance of 360 light-years.

Star chart in white with black dots for stars showing cross shape at center.
The stars of Crux the Southern Cross. Image via/ IAU/ Sky and Telescope/ Wikimedia Commons.

Use the Southern Cross to find due south

Arrows coming from the Southern Cross and Archernar meet in the middle, where the South Celestial Pole is.
Method #1. The south celestial pole is located halfway between Gacrux, the head of the Southern Cross, and the bright star Achernar. For a practical trick, place one hand at the Cross and the other at Achernar. Now bring them together in a clap! Your hands should meet right at the south celestial pole. Chart via EarthSky.
Arrows from the Southern Cross and Alpha Centauri converge at the south celestial pole.
Method #2. Draw an imaginary line extending the long axis of the Southern Cross, and another one bisecting the 2 “Pointer Stars,” Alpha and Beta Centauri. The south celestial pole lies at the intersection between those 2 lines. Chart via EarthSky.
Arrow, divided into 4 segments each equal to the length of the Southern Cross, from the cross to the south celestial pole.
Method #3. To locate the south celestial pole, extend the long axis of the Southern Cross from the head of the cross through its foot, 4 times its own length. Chart via EarthSky.

The Jewel Box and other clusters in Crux

The Jewel Box is one of the most beautiful open clusters in the Southern Hemisphere. It lies just 1 degree from Beta Crucis. The Jewel Box, or NGC 4755, is bright at magnitude 4.2. Kappa Crucis, a magnitude 5.89 star, lies inside.

You can see the Jewel Box without optical aid. But a pair of binoculars or a telescope will bring more of the stars into focus.

Can you see color differences between these glittering gems?

Glittering cluster of mostly blue stars with one red one near center.
NGC 4755, or the Jewel Box, from ESO’s La Silla Observatory. Image via ESO.

The Coalsack Nebula

The easiest dark nebula to see in the sky is the Coalsack Nebula, found in the southeastern corner of Crux. The Coalsack is a dark, cloudy patch of dust and gas that obscures an entire swath of the Milky Way’s stars that lies behind it.

Large irregular black area surrounded by starfield and bright blue star at top.
Meet the Coalsack, a huge cloud of gas and dust in space. The dust in this and other dark nebulae absorb and scatter the light of background stars. This creates a region of the sky that looks starless, but it’s really a place where new stars are forming. May is one of the best months to see the Coalsack in the constellation Crux in the Southern Hemisphere. This image is from the Wide Field Imager on the MPG/ESO 2.2-meter telescope. Image via ESO.

Bottom line: Crux, the constellation of the Southern Cross, is a hallmark of southern skies and contains the open cluster known as the Jewel Box.

Read more: How to see the Southern Cross from the Northern Hemisphere

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Joplin tornado: 15-year anniversary of a disaster

Joplin tornado damage with shredded houses all up and down a street with one vehicle in the street.
In this image from 10 days after the May 22, 2011, EF5 tornado that hit Joplin, Missouri, piles of rubble mark where people’s homes once stood. It’s now been 15 years since the Joplin tornado, which killed 158 people directly and 5 through a deadly fungus it stirred up. Image via Bob Webster/ Wikimedia Commons.

The 15-year anniversary of the deadly Joplin tornado

On May 22, 2011, an EF5 tornado with winds of more than 200 miles (322 km) per hour devastated Joplin, Missouri. It was the 7th-deadliest tornado in the U.S. and the deadliest tornado since 1947. As the tornado bulldozed a path nearly a mile wide through the city, it took the lives of 158 people and injured more than 1,000.

And, in the days that followed, five more people died due to a deadly soil-dwelling fungus the tornado stirred up.

The Joplin tornado flattened homes, schools and businesses. It caused catastrophic damage at a nine-story hospital, St. John’s Regional Medical Center, which would later have to be demolished. And it became the costliest tornado in U.S. history at the time, with damages approaching $3 billion.

10-story rectangular building with windows blown out and much interior damage, near completely destroyed building.
The Joplin tornado damaged St. John’s Hospital beyond repair. Today, a new hospital stands by the interstate. Image via Interlati/ Wikimedia Commons.

A hesitancy to act

The tornado struck on a Sunday evening. A local high school had just finished graduation ceremonies, plus other people were out and about, wrapping up their weekends. Due to the high death toll, the National Weather Service (NWS) conducted a service assessment to try to understand why so many people died.

On the one hand, the NWS found that many of the homes that were in the path of the tornado were poorly constructed. In fact, fatalities occurred in 59 different homes. There were also 19 deaths at a nursing home, four at an ICU, 11 in churches and eight in a Home Depot.

But another finding by the NWS was that when the tornado sirens first went off, many people were initially complacent. Instead of reacting at the first warning, many people reported that they waited as they assessed the risk and looked for more confirmation.

For many, confirmation came in the form of black skies and a terrifying roar as the rain-wrapped tornado overtook them.

Netflix made an excellent documentary on the Joplin tornado called The Twister: Caught in the Storm.

After the tornado, the killer fungus

As the city came together to clean up and mourn the dead, a new lethal aspect of the tornado came to light. While treating the injured in the following days, doctors noticed some survivors were developing severe infections in their wounds.

The culprit turned out to be a rare and often lethal fungal infection. The fungal spores were mucormycetes. Normally, they live in soil and decaying plant matter. But the violent tornado scoured the ground, ripping off topsoil and throwing the dirt and debris into the air. For some people, this dirt became deeply embedded in their wounds.

A 2013 study found that 13 people were affected by the fungus, and five of them died. The fungus can cause flesh-eating infections. The study said:

The researchers discovered a significant link between fungal infection and the occurrence of penetrating wounds (especially multiple wounds) containing wood, soil, gravel, and other foreign bodies.

Joplin today

Today, much of the city of Joplin has been rebuilt. At the site of the former hospital a park now stands. And the new hospital, Mercy Hospital Joplin, stands alongside Interstate 44.

The six schools that were destroyed have now been rebuilt. While many homes replaced those that were turned to rubble, there are still some empty lots. Those lots, and the lack of mature trees, mean you can still see the path of the Joplin tornado on satellite even after 15 years.

Satellite view of a city with a light brown path through the streets and otherwise green trees.
This was the satellite view of Joplin, Missouri, in 2011 following the May 22 tornado. Image via NOAA.
Satellite view of a city with roads and dark green trees plus a lighter tan strip.
This is the satellite view of Joplin, Missouri, today. You can still see a lighter brown strip where the tornado destroyed buildings and trees, changing the landscape. Image via Google Earth Pro.

Bottom line: It’s been 15 years since the Joplin tornado killed more than 150 people. What is the town of Joplin, Missouri, like today?

Read more: The Enhanced Fujita Scale rates the strength of a tornado

Science news, night sky events and beautiful photos, all in one place. Click here to subscribe to our free daily newsletter.

The post Joplin tornado: 15-year anniversary of a disaster first appeared on EarthSky.



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Joplin tornado damage with shredded houses all up and down a street with one vehicle in the street.
In this image from 10 days after the May 22, 2011, EF5 tornado that hit Joplin, Missouri, piles of rubble mark where people’s homes once stood. It’s now been 15 years since the Joplin tornado, which killed 158 people directly and 5 through a deadly fungus it stirred up. Image via Bob Webster/ Wikimedia Commons.

The 15-year anniversary of the deadly Joplin tornado

On May 22, 2011, an EF5 tornado with winds of more than 200 miles (322 km) per hour devastated Joplin, Missouri. It was the 7th-deadliest tornado in the U.S. and the deadliest tornado since 1947. As the tornado bulldozed a path nearly a mile wide through the city, it took the lives of 158 people and injured more than 1,000.

And, in the days that followed, five more people died due to a deadly soil-dwelling fungus the tornado stirred up.

The Joplin tornado flattened homes, schools and businesses. It caused catastrophic damage at a nine-story hospital, St. John’s Regional Medical Center, which would later have to be demolished. And it became the costliest tornado in U.S. history at the time, with damages approaching $3 billion.

10-story rectangular building with windows blown out and much interior damage, near completely destroyed building.
The Joplin tornado damaged St. John’s Hospital beyond repair. Today, a new hospital stands by the interstate. Image via Interlati/ Wikimedia Commons.

A hesitancy to act

The tornado struck on a Sunday evening. A local high school had just finished graduation ceremonies, plus other people were out and about, wrapping up their weekends. Due to the high death toll, the National Weather Service (NWS) conducted a service assessment to try to understand why so many people died.

On the one hand, the NWS found that many of the homes that were in the path of the tornado were poorly constructed. In fact, fatalities occurred in 59 different homes. There were also 19 deaths at a nursing home, four at an ICU, 11 in churches and eight in a Home Depot.

But another finding by the NWS was that when the tornado sirens first went off, many people were initially complacent. Instead of reacting at the first warning, many people reported that they waited as they assessed the risk and looked for more confirmation.

For many, confirmation came in the form of black skies and a terrifying roar as the rain-wrapped tornado overtook them.

Netflix made an excellent documentary on the Joplin tornado called The Twister: Caught in the Storm.

After the tornado, the killer fungus

As the city came together to clean up and mourn the dead, a new lethal aspect of the tornado came to light. While treating the injured in the following days, doctors noticed some survivors were developing severe infections in their wounds.

The culprit turned out to be a rare and often lethal fungal infection. The fungal spores were mucormycetes. Normally, they live in soil and decaying plant matter. But the violent tornado scoured the ground, ripping off topsoil and throwing the dirt and debris into the air. For some people, this dirt became deeply embedded in their wounds.

A 2013 study found that 13 people were affected by the fungus, and five of them died. The fungus can cause flesh-eating infections. The study said:

The researchers discovered a significant link between fungal infection and the occurrence of penetrating wounds (especially multiple wounds) containing wood, soil, gravel, and other foreign bodies.

Joplin today

Today, much of the city of Joplin has been rebuilt. At the site of the former hospital a park now stands. And the new hospital, Mercy Hospital Joplin, stands alongside Interstate 44.

The six schools that were destroyed have now been rebuilt. While many homes replaced those that were turned to rubble, there are still some empty lots. Those lots, and the lack of mature trees, mean you can still see the path of the Joplin tornado on satellite even after 15 years.

Satellite view of a city with a light brown path through the streets and otherwise green trees.
This was the satellite view of Joplin, Missouri, in 2011 following the May 22 tornado. Image via NOAA.
Satellite view of a city with roads and dark green trees plus a lighter tan strip.
This is the satellite view of Joplin, Missouri, today. You can still see a lighter brown strip where the tornado destroyed buildings and trees, changing the landscape. Image via Google Earth Pro.

Bottom line: It’s been 15 years since the Joplin tornado killed more than 150 people. What is the town of Joplin, Missouri, like today?

Read more: The Enhanced Fujita Scale rates the strength of a tornado

Science news, night sky events and beautiful photos, all in one place. Click here to subscribe to our free daily newsletter.

The post Joplin tornado: 15-year anniversary of a disaster first appeared on EarthSky.



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Meet Regulus, Leo the Lion’s Heart and brightest star

Star chart: animal-shaped constellation with head at right side and bright star, Regulus, in chest area.
Leo the Lion’s brightest star is Regulus, aka the Lion’s Heart. Regulus marks the bright dot at the bottom of a backward question mark that forms Leo’s head and shoulders. This pattern is called the Sickle. An easily identifiable triangle depicts the Lion’s hindquarters and tail, with the star Denebola marking the tail of the Lion. Chart via EarthSky.

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Regulus is the brightest star in the constellation Leo the Lion. Also known as Alpha Leonis, it ranks 21st in the list of brightest stars in our sky.

It’s located near the ecliptic, or sun’s path across our sky. So both Earth’s Northern and Southern Hemispheres see Regulus equally well.

Regulus is part of a backward question mark star pattern, and it marks the dot at the bottom of the question mark. This pattern, known as the Sickle, makes up the head and forequarters of Leo the Lion.

You’ll recognize Regulus for its brightness and blue-white color. It looks like one star to the eye, but it’s really four stars (that we know of so far).

Regulus is located about 79 light-years from Earth.

Star chart with stars in black on white and labeled, along with several labeled Messier objects.
A star chart showing the constellation Leo the Lion. On the right is a pattern that looks like a flipped question mark, the Sickle. This is the most recognizable pattern to look for when trying to locate Leo in the sky. Image via Torsten Bronger/ Wikimedia Commons.

Finding the Lion from the Northern Hemisphere

In the Northern Hemisphere, the star Regulus and its constellation Leo the Lion are harbingers of spring.

They crept higher in the sky with each passing day in March and April, as northern winter favorites – like Orion the Hunter – descended westward.

And now, in May, blue-white Regulus is brilliant in the eastern evening sky as soon as the sun goes down.

And a darker sky reveals the distinctive Sickle and the overall shape of the Lion.

From the Northern Hemisphere, Regulus is visible at some time of night throughout the year, except for about a month on either side of August 22. If you looked toward Regulus around that date, you’d see the sun.

In the Northern Hemisphere, Regulus is known as one of three bright stars making up the asterism of the Spring Triangle.

From the Southern Hemisphere, the Lion is upside down

Via Daniel Gaussen, Founder & Guide – Stargaze Mackenzie – New Zealand

From southern latitudes, the figure of the Lion – named long ago by stargazers on the northern part of Earth’s globe – appears upside down. Regulus traditionally marks Leo’s lower front paw. But Regulus appears as the highest of Leo’s stars from our southerly perspective.

And, from our latitudes on the south of Earth’s globe, the Sickle asterism appears as a mirrored upside-down question mark. This pattern is clearly recognizable for skywatchers tracing the inverted Lion across the northern sky.

As seen from either the Northern or Southern Hemisphere, Regulus more or less follows the sun and moon’s path across our sky. So those in the Northern Hemisphere face generally southward to see Regulus make its wide arc across the sky. But we in the Southern Hemisphere face generally northward to see it.

At a latitude of 35 degrees south, Regulus climbs to about 43 degrees above the northern horizon at its highest. It’s noticeably higher than other bright northern stars, such as Vega. In the Southern Hemisphere, Regulus is one of the easier northern stars to spot during the southern autumn and early winter evenings (May through August).

So, while Leo is a northern constellation, its most prominent marker – Regulus – remains a useful and reliable reference point from the Southern Hemisphere during the colder months.

Despite the constellation’s inverted appearance, the clarity of Regulus and the distinctive Sickle pattern make Leo surprisingly easy to identify once you know what to look for.

Planets and the moon pass near it

Regulus is the only 1st magnitude star to sit almost squarely on the ecliptic, or path of the sun, moon and planets across our sky.

So the moon sweeps past Regulus once a month when this star is visible. In some years, the moon occults – or passes in front of – Regulus as seen from Earth. We’re in a series of 20 lunar occultations of Regulus now, lasting from July 2025 to December 2026. During the December 2026 occultation, Mars and Jupiter will be nearby.

And bright planets also sometimes pass Regulus. Planets can even sometimes occult – or pass in front of – this star. The last planet to occult Regulus was Venus on July 7, 1959. Then on October 1, 2044, Venus will occult Regulus again.

Don’t miss a thing! Visit our monthly night sky guide.

A blue, egg-shaped star

Regulus is a multiple star system, consisting of at least four stars. The main star – Regulus A – is large and blue with a spectral type of B8 IVn. Its surface temperature averages about 12,460 kelvin (21,970 degrees F or 12,190 degrees C), which is much higher than our sun’s surface temperature. Regulus A is 3.8 times the mass of our sun, about 4 times as wide, and almost 300 times as bright.

Regulus A spins on its axis once every 16 hours. In contrast, our sun spins on its axis about once every 27 days. This fast rotation causes Regulus A to bulge at its equator, so it appears oblate, or egg-shaped. In fact, if Regulus rotated just a bit faster, it would fly apart!

And Regulus isn’t the only star with a fast spin. The stars Altair and Achernar are also fast spinners with flattened, oblate shapes.

An egg-shaped spheroid with a much smaller sphere at the lower right.
Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) created this computer-generated model of Regulus in 2005. Next to it there is a model of our sun for scale. The high rotation rate of Regulus creates pronounced equatorial bulging, such that its diameter across its equator (running nearly vertically in this image) is 1/3 longer than its north-south diameter. Image via Wenjin Huang/ Georgia State University/ NOIRlab.

We can see 3 of Regulus’ 4 stars

Look through a small telescope using at least 50x magnification, and you will see Regulus as two objects separated by 177 arcseconds. The brighter of the pair is Regulus A.

The fainter one is Regulus B, a cool “orange” dwarf star with a spectral classification of K2 V. The B star has a mass that is 80% of the sun’s, and it’s half as bright. It has a surface temperature of 4,885 kelvin (8,300 F or 4,600 C), and it shines at magnitude 8.1.

Regulus B has its own companion: Regulus C. At magnitude 13.5, it’s only visible with powerful telescopes. With just 1/3 the mass of the sun, Regulus C is a red dwarf star with a spectral classification of M4 V. Regulus B and C are gravitationally bound to each other, and together they’re called Regulus BC. The distances between B and C ranged from 4.0 to 2.5 arcseconds between 1867 and 1943. There are no recently available measurements.

The 4th star in the system has never been directly resolved via imaging. But its presence is revealed by spectroscopic analysis of Regulus A. Astronomers think it may be a closely orbiting white dwarf star.

You might have heard of a star called Regulus D. This doesn’t refer to the spectroscopic companion of Regulus A, but to a 12th-magnitude star that sits 212 arcseconds from Regulus. For decades, people believed it to be a companion of Regulus, but recent studies from the Gaia satellite show this to be a background star not related to the Regulus system.

A rex by any other name

The name Regulus is from the diminutive form of the Latin rex, meaning little king.

Ancient Arab stargazers called Regulus by the name Qalb al-Asad, which means Heart of the Lion. It also bears the nickname Cor Leonis, again meaning Lion’s Heart. Fittingly, King Richard I of England was also famously known as the Lionheart, or more commonly Coeur de Lion in French.

There is a great deal of mythology associated with Leo, perhaps the most common tale being that Leo was the Nemean Lion of the Hercules story. Some Peruvians also knew these stars as the Mountain Lion, whereas in China it was sometimes seen as a horse, and at other times as part of a dragon. Christians in the Middle Ages sometimes referred to it as one of Daniel’s lions.

Antique colored etching of two yellow lions, one much larger, with the constellations' stars superimposed.
The larger lion is the constellation Leo, with the star Regulus at its heart, as depicted on a set of constellation cards, Urania’s Mirror, published in London in 1825. Above it is the faint constellation Leo Minor. Image via Library of Congress/ Wikimedia Commons.

A galaxy photobombs Regulus

Situated 1/3 degree north of Regulus is the galaxy Leo I. You can see it as a faint patch of light in the photo below. Leo I is difficult to see due to its proximity to Regulus. Albert George Wilson found it on photographic plates taken as part of the National Geographic Society-Palomar Observatory Sky Survey in 1950. It would be another 40 years before anyone viewed it.

Leo I is a dwarf galaxy, and a member of our local group. Amateur astronomers can view it, but this requires dark skies and a large telescope.

In a field of stars, a large, brilliant blue-white star. Above it is a faint horizontal oval smudge of light.
Regulus as photographed using a telescope. The faint smudge above it is the dwarf galaxy Leo I. Image via Fred Espenak. Used with permission.

Bottom line: Regulus, the brightest star in the constellation Leo the Lion, is associated with the arrival of spring and is prominent in May skies. It looks like a single point of light, but is really four stars.

Summer Triangle star: Altair is variable and spins fast!

What is the Sickle in Leo?

The post Meet Regulus, Leo the Lion’s Heart and brightest star first appeared on EarthSky.



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Star chart: animal-shaped constellation with head at right side and bright star, Regulus, in chest area.
Leo the Lion’s brightest star is Regulus, aka the Lion’s Heart. Regulus marks the bright dot at the bottom of a backward question mark that forms Leo’s head and shoulders. This pattern is called the Sickle. An easily identifiable triangle depicts the Lion’s hindquarters and tail, with the star Denebola marking the tail of the Lion. Chart via EarthSky.

Don’t miss the next unmissable night sky event. Sign up for our free newsletter for daily night sky updates, as well as the latest science news.

Regulus is the brightest star in the constellation Leo the Lion. Also known as Alpha Leonis, it ranks 21st in the list of brightest stars in our sky.

It’s located near the ecliptic, or sun’s path across our sky. So both Earth’s Northern and Southern Hemispheres see Regulus equally well.

Regulus is part of a backward question mark star pattern, and it marks the dot at the bottom of the question mark. This pattern, known as the Sickle, makes up the head and forequarters of Leo the Lion.

You’ll recognize Regulus for its brightness and blue-white color. It looks like one star to the eye, but it’s really four stars (that we know of so far).

Regulus is located about 79 light-years from Earth.

Star chart with stars in black on white and labeled, along with several labeled Messier objects.
A star chart showing the constellation Leo the Lion. On the right is a pattern that looks like a flipped question mark, the Sickle. This is the most recognizable pattern to look for when trying to locate Leo in the sky. Image via Torsten Bronger/ Wikimedia Commons.

Finding the Lion from the Northern Hemisphere

In the Northern Hemisphere, the star Regulus and its constellation Leo the Lion are harbingers of spring.

They crept higher in the sky with each passing day in March and April, as northern winter favorites – like Orion the Hunter – descended westward.

And now, in May, blue-white Regulus is brilliant in the eastern evening sky as soon as the sun goes down.

And a darker sky reveals the distinctive Sickle and the overall shape of the Lion.

From the Northern Hemisphere, Regulus is visible at some time of night throughout the year, except for about a month on either side of August 22. If you looked toward Regulus around that date, you’d see the sun.

In the Northern Hemisphere, Regulus is known as one of three bright stars making up the asterism of the Spring Triangle.

From the Southern Hemisphere, the Lion is upside down

Via Daniel Gaussen, Founder & Guide – Stargaze Mackenzie – New Zealand

From southern latitudes, the figure of the Lion – named long ago by stargazers on the northern part of Earth’s globe – appears upside down. Regulus traditionally marks Leo’s lower front paw. But Regulus appears as the highest of Leo’s stars from our southerly perspective.

And, from our latitudes on the south of Earth’s globe, the Sickle asterism appears as a mirrored upside-down question mark. This pattern is clearly recognizable for skywatchers tracing the inverted Lion across the northern sky.

As seen from either the Northern or Southern Hemisphere, Regulus more or less follows the sun and moon’s path across our sky. So those in the Northern Hemisphere face generally southward to see Regulus make its wide arc across the sky. But we in the Southern Hemisphere face generally northward to see it.

At a latitude of 35 degrees south, Regulus climbs to about 43 degrees above the northern horizon at its highest. It’s noticeably higher than other bright northern stars, such as Vega. In the Southern Hemisphere, Regulus is one of the easier northern stars to spot during the southern autumn and early winter evenings (May through August).

So, while Leo is a northern constellation, its most prominent marker – Regulus – remains a useful and reliable reference point from the Southern Hemisphere during the colder months.

Despite the constellation’s inverted appearance, the clarity of Regulus and the distinctive Sickle pattern make Leo surprisingly easy to identify once you know what to look for.

Planets and the moon pass near it

Regulus is the only 1st magnitude star to sit almost squarely on the ecliptic, or path of the sun, moon and planets across our sky.

So the moon sweeps past Regulus once a month when this star is visible. In some years, the moon occults – or passes in front of – Regulus as seen from Earth. We’re in a series of 20 lunar occultations of Regulus now, lasting from July 2025 to December 2026. During the December 2026 occultation, Mars and Jupiter will be nearby.

And bright planets also sometimes pass Regulus. Planets can even sometimes occult – or pass in front of – this star. The last planet to occult Regulus was Venus on July 7, 1959. Then on October 1, 2044, Venus will occult Regulus again.

Don’t miss a thing! Visit our monthly night sky guide.

A blue, egg-shaped star

Regulus is a multiple star system, consisting of at least four stars. The main star – Regulus A – is large and blue with a spectral type of B8 IVn. Its surface temperature averages about 12,460 kelvin (21,970 degrees F or 12,190 degrees C), which is much higher than our sun’s surface temperature. Regulus A is 3.8 times the mass of our sun, about 4 times as wide, and almost 300 times as bright.

Regulus A spins on its axis once every 16 hours. In contrast, our sun spins on its axis about once every 27 days. This fast rotation causes Regulus A to bulge at its equator, so it appears oblate, or egg-shaped. In fact, if Regulus rotated just a bit faster, it would fly apart!

And Regulus isn’t the only star with a fast spin. The stars Altair and Achernar are also fast spinners with flattened, oblate shapes.

An egg-shaped spheroid with a much smaller sphere at the lower right.
Georgia State University’s Center for High Angular Resolution Astronomy (CHARA) created this computer-generated model of Regulus in 2005. Next to it there is a model of our sun for scale. The high rotation rate of Regulus creates pronounced equatorial bulging, such that its diameter across its equator (running nearly vertically in this image) is 1/3 longer than its north-south diameter. Image via Wenjin Huang/ Georgia State University/ NOIRlab.

We can see 3 of Regulus’ 4 stars

Look through a small telescope using at least 50x magnification, and you will see Regulus as two objects separated by 177 arcseconds. The brighter of the pair is Regulus A.

The fainter one is Regulus B, a cool “orange” dwarf star with a spectral classification of K2 V. The B star has a mass that is 80% of the sun’s, and it’s half as bright. It has a surface temperature of 4,885 kelvin (8,300 F or 4,600 C), and it shines at magnitude 8.1.

Regulus B has its own companion: Regulus C. At magnitude 13.5, it’s only visible with powerful telescopes. With just 1/3 the mass of the sun, Regulus C is a red dwarf star with a spectral classification of M4 V. Regulus B and C are gravitationally bound to each other, and together they’re called Regulus BC. The distances between B and C ranged from 4.0 to 2.5 arcseconds between 1867 and 1943. There are no recently available measurements.

The 4th star in the system has never been directly resolved via imaging. But its presence is revealed by spectroscopic analysis of Regulus A. Astronomers think it may be a closely orbiting white dwarf star.

You might have heard of a star called Regulus D. This doesn’t refer to the spectroscopic companion of Regulus A, but to a 12th-magnitude star that sits 212 arcseconds from Regulus. For decades, people believed it to be a companion of Regulus, but recent studies from the Gaia satellite show this to be a background star not related to the Regulus system.

A rex by any other name

The name Regulus is from the diminutive form of the Latin rex, meaning little king.

Ancient Arab stargazers called Regulus by the name Qalb al-Asad, which means Heart of the Lion. It also bears the nickname Cor Leonis, again meaning Lion’s Heart. Fittingly, King Richard I of England was also famously known as the Lionheart, or more commonly Coeur de Lion in French.

There is a great deal of mythology associated with Leo, perhaps the most common tale being that Leo was the Nemean Lion of the Hercules story. Some Peruvians also knew these stars as the Mountain Lion, whereas in China it was sometimes seen as a horse, and at other times as part of a dragon. Christians in the Middle Ages sometimes referred to it as one of Daniel’s lions.

Antique colored etching of two yellow lions, one much larger, with the constellations' stars superimposed.
The larger lion is the constellation Leo, with the star Regulus at its heart, as depicted on a set of constellation cards, Urania’s Mirror, published in London in 1825. Above it is the faint constellation Leo Minor. Image via Library of Congress/ Wikimedia Commons.

A galaxy photobombs Regulus

Situated 1/3 degree north of Regulus is the galaxy Leo I. You can see it as a faint patch of light in the photo below. Leo I is difficult to see due to its proximity to Regulus. Albert George Wilson found it on photographic plates taken as part of the National Geographic Society-Palomar Observatory Sky Survey in 1950. It would be another 40 years before anyone viewed it.

Leo I is a dwarf galaxy, and a member of our local group. Amateur astronomers can view it, but this requires dark skies and a large telescope.

In a field of stars, a large, brilliant blue-white star. Above it is a faint horizontal oval smudge of light.
Regulus as photographed using a telescope. The faint smudge above it is the dwarf galaxy Leo I. Image via Fred Espenak. Used with permission.

Bottom line: Regulus, the brightest star in the constellation Leo the Lion, is associated with the arrival of spring and is prominent in May skies. It looks like a single point of light, but is really four stars.

Summer Triangle star: Altair is variable and spins fast!

What is the Sickle in Leo?

The post Meet Regulus, Leo the Lion’s Heart and brightest star first appeared on EarthSky.



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2026 name list for Atlantic hurricanes: Is yours among them?

Hurricanes: Satellite image of hurricane with 2026 hurricane names on top.
This is the list of tropical cyclone names for the 2026 Atlantic hurricane season. Read about the names of hurricanes below.

Read: NOAA’s hurricane season forecast for 2026

Atlantic hurricane names for 2026

NOAA’s Climate Prediction Center has just released its hurricane season outlook for 2026. But what are the names for the 2026 Atlantic tropical cyclones and hurricanes?

See the complete list of 2026 tropical cyclone and hurricane names in the image above. If any of these storms become truly destructive in 2026, the World Meteorological Organization, which is in charge of the list, retires and replaces the name. For example, in 2024, the World Meteorological Organization retired the names Beryl, Helene and Milton. Helene, in particular, became the deadliest storm in the U.S. since Katrina in 2005.

The 2026 Atlantic hurricane season officially starts June 1 and extends through November 30.

If you live near the Atlantic basin, you can keep up-to-date with forecasts from the National Hurricane Center.

Learn more about how to prepare for hurricane season.

How do hurricanes get their names?

Meteorologists long ago learned that naming tropical storms and hurricanes helps people remember the storms, communicate about them more effectively, and consequently stay safer if and when a particular storm strikes a coast.

These experts assign names to tropical storms according to an approved list before the start of each hurricane season. The U.S. National Hurricane Center started this practice in the early 1950s. Now, the World Meteorological Organization (WMO) generates and maintains the list of hurricane names.

Here are the hurricane names for 2026

Atlantic hurricane names (season runs from June 1 to November 30) are: Arthur, Bertha, Cristobal, Dolly, Edouard, Fay, Gonzalo, Hanna, Isaias, Josephine, Kyle. Leah, Marco, Nana, Omar. Paulette, Rene, Sally, Teddy, Vicky and Wilfred.

Eastern North Pacific hurricane names (season runs from May 15 to November 30) are: Amanda, Boris, Cristina, Douglas, Elida, Fausto, Genevieve, Hernan, Iselle, Julio, Karina, Lowell, Marie, Norbert, Odalys, Polo, Rachel, Simon, Trudy, Vance, Winnie. Xavier, Yolanda and Zeke.

If you’re interested, you can view those names, and names for upcoming years, at the U.S. National Hurricane Center.

Gif showing swirling white clouds over Florida's center moving northeast.
In 2022, Hurricane Ian devastated Florida’s Gulf Coast. It also brought flooding to central Florida, ripped roofs off on the Atlantic Coast and then menaced South Carolina. The name Ian will never again be used for a tropical cyclone or hurricane. Image via NOAA/ GOES.

The history of hurricane names

While people have been naming major storms for hundreds of years, most hurricanes originally had a designation using a system of latitude-longitude numbers. This was useful to meteorologists trying to track these storms. Unfortunately, this system confused people living on coasts seeking hurricane information.

In the early 1950s, the U.S. National Hurricane Center first developed a formal practice for storm naming for the Atlantic Ocean. At that time, storms got their names according to a phonetic alphabet (e.g., Able, Baker, Charlie) and the names used were the same for each hurricane season. In other words, the first hurricane of a season was always named “Able,” the second “Baker,” and so on.

In 1953, to avoid the repetitive use of names, the National Weather Service revised the system to give storms female names. By doing this, the National Weather Service was mimicking the habit of naval meteorologists, who named the storms after women, much as ships at sea traditionally had female names.

In 1978–1979, they revised the system again to include both female and male hurricane names.

See the complete history of naming hurricanes, including retired names, from NOAA.

When does a storm receive a name?

Tropical storms get a name when they display a rotating circulation pattern and wind speeds reach 39 miles per hour (63 kilometers per hour). A tropical storm develops into a hurricane when wind speeds go above 74 mph (119 km/h).

Experts have developed lists of hurricane names for many of the major ocean basins around the world. Today, there are six lists of hurricane names in use for Atlantic Ocean and Eastern North Pacific storms. These lists rotate, one each year. So that means the list of this year’s hurricane names for each basin will come up again six years from now.

However, there’s an exception to this practice. The World Meteorological Organization retires the names of extremely damaging hurricanes for legal, cultural sensitivity and historical reasons. For example, they retired the name Katrina in 2005 following the devastating impact that Hurricane Katrina had on New Orleans. In 2022, the World Meteorological Organization Hurricane Committee retired the names Fiona and Ian.

Large round white hurricane seen from above, with distinct spirals and eye, in Gulf of Mexico with green land areas visible.
Hurricane Katrina on August 28, 2005. Image via NASA.

Bottom line: The forecasts for Atlantic hurricanes and tropical storms is out. And the hurricane names for 2026 are ready. What’ll happen next?

Read: NOAA’s hurricane season forecast for 2026

Read more: What is a hurricane storm surge?

The post 2026 name list for Atlantic hurricanes: Is yours among them? first appeared on EarthSky.



from EarthSky https://ift.tt/0lK3YCe
Hurricanes: Satellite image of hurricane with 2026 hurricane names on top.
This is the list of tropical cyclone names for the 2026 Atlantic hurricane season. Read about the names of hurricanes below.

Read: NOAA’s hurricane season forecast for 2026

Atlantic hurricane names for 2026

NOAA’s Climate Prediction Center has just released its hurricane season outlook for 2026. But what are the names for the 2026 Atlantic tropical cyclones and hurricanes?

See the complete list of 2026 tropical cyclone and hurricane names in the image above. If any of these storms become truly destructive in 2026, the World Meteorological Organization, which is in charge of the list, retires and replaces the name. For example, in 2024, the World Meteorological Organization retired the names Beryl, Helene and Milton. Helene, in particular, became the deadliest storm in the U.S. since Katrina in 2005.

The 2026 Atlantic hurricane season officially starts June 1 and extends through November 30.

If you live near the Atlantic basin, you can keep up-to-date with forecasts from the National Hurricane Center.

Learn more about how to prepare for hurricane season.

How do hurricanes get their names?

Meteorologists long ago learned that naming tropical storms and hurricanes helps people remember the storms, communicate about them more effectively, and consequently stay safer if and when a particular storm strikes a coast.

These experts assign names to tropical storms according to an approved list before the start of each hurricane season. The U.S. National Hurricane Center started this practice in the early 1950s. Now, the World Meteorological Organization (WMO) generates and maintains the list of hurricane names.

Here are the hurricane names for 2026

Atlantic hurricane names (season runs from June 1 to November 30) are: Arthur, Bertha, Cristobal, Dolly, Edouard, Fay, Gonzalo, Hanna, Isaias, Josephine, Kyle. Leah, Marco, Nana, Omar. Paulette, Rene, Sally, Teddy, Vicky and Wilfred.

Eastern North Pacific hurricane names (season runs from May 15 to November 30) are: Amanda, Boris, Cristina, Douglas, Elida, Fausto, Genevieve, Hernan, Iselle, Julio, Karina, Lowell, Marie, Norbert, Odalys, Polo, Rachel, Simon, Trudy, Vance, Winnie. Xavier, Yolanda and Zeke.

If you’re interested, you can view those names, and names for upcoming years, at the U.S. National Hurricane Center.

Gif showing swirling white clouds over Florida's center moving northeast.
In 2022, Hurricane Ian devastated Florida’s Gulf Coast. It also brought flooding to central Florida, ripped roofs off on the Atlantic Coast and then menaced South Carolina. The name Ian will never again be used for a tropical cyclone or hurricane. Image via NOAA/ GOES.

The history of hurricane names

While people have been naming major storms for hundreds of years, most hurricanes originally had a designation using a system of latitude-longitude numbers. This was useful to meteorologists trying to track these storms. Unfortunately, this system confused people living on coasts seeking hurricane information.

In the early 1950s, the U.S. National Hurricane Center first developed a formal practice for storm naming for the Atlantic Ocean. At that time, storms got their names according to a phonetic alphabet (e.g., Able, Baker, Charlie) and the names used were the same for each hurricane season. In other words, the first hurricane of a season was always named “Able,” the second “Baker,” and so on.

In 1953, to avoid the repetitive use of names, the National Weather Service revised the system to give storms female names. By doing this, the National Weather Service was mimicking the habit of naval meteorologists, who named the storms after women, much as ships at sea traditionally had female names.

In 1978–1979, they revised the system again to include both female and male hurricane names.

See the complete history of naming hurricanes, including retired names, from NOAA.

When does a storm receive a name?

Tropical storms get a name when they display a rotating circulation pattern and wind speeds reach 39 miles per hour (63 kilometers per hour). A tropical storm develops into a hurricane when wind speeds go above 74 mph (119 km/h).

Experts have developed lists of hurricane names for many of the major ocean basins around the world. Today, there are six lists of hurricane names in use for Atlantic Ocean and Eastern North Pacific storms. These lists rotate, one each year. So that means the list of this year’s hurricane names for each basin will come up again six years from now.

However, there’s an exception to this practice. The World Meteorological Organization retires the names of extremely damaging hurricanes for legal, cultural sensitivity and historical reasons. For example, they retired the name Katrina in 2005 following the devastating impact that Hurricane Katrina had on New Orleans. In 2022, the World Meteorological Organization Hurricane Committee retired the names Fiona and Ian.

Large round white hurricane seen from above, with distinct spirals and eye, in Gulf of Mexico with green land areas visible.
Hurricane Katrina on August 28, 2005. Image via NASA.

Bottom line: The forecasts for Atlantic hurricanes and tropical storms is out. And the hurricane names for 2026 are ready. What’ll happen next?

Read: NOAA’s hurricane season forecast for 2026

Read more: What is a hurricane storm surge?

The post 2026 name list for Atlantic hurricanes: Is yours among them? first appeared on EarthSky.



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