All you need to know: 2019’s Leonid meteor shower

Round overexposed moon and long thin white streak.

This isn’t a Leonid meteor. It’s an Orionid. But – as this photo shows – you can sometimes catch a meteor in bright moonlight, assuming it’s bright enough. Photo taken in late October 2016 by Eliot Herman in Tucson, Arizona. Thanks, Eliot!

November’s wonderful Leonid meteor shower is active from about November 6 to 30 each year. The peak is expected in 2019 on the night of November 17 (morning of November 18). The shower happens as our world crosses the orbital path of Comet 55P/Tempel-Tuttle. Like many comets, Tempel-Tuttle litters its orbit with bits of debris. It’s when this cometary debris enters Earth’s atmosphere and vaporizes that we see the Leonid meteor shower. In 2019, a waning gibbous moon will light up the sky during the shower’s peak. In a dark sky, absent of moonlight, you can see up to 10 to 15 meteors per hour at the peak. In 2019’s moonlit sky? We can’t predict, but some of the brighter meteors should be visible in moonlight.

Although this shower is known for its periodic storms, no Leonid storm is expected this year. Keep reading to learn more.

The 2019 lunar calendars are here! Order yours before they’re gone. Makes a great gift.

Thin white almost vertical streak over dark, distant hilly horizon.

James Younger sent in this photo during the 2015 peak of the Leonid meteor shower. It’s a meteor over the San Juan Islands in the Pacific Northwest, between the U.S. mainland and Vancouver Island, British Columbia.

How many Leonid meteors will you see in 2019? The answer always depends on when you watch, where you watch, and on the clarity and darkness of your night sky.

In 2019, no matter where you are on Earth – and no matter when you watch, on the morning of the peak itself, or on the morning leading up to the peak – the best hours of the night for meteor-watching will be hindered by the bright moon. Those hours are between midnight and dawn, when Earth’s forward motion through space has carried your part of Earth head-on into the meteor stream.

Also in 2019, there’s really no way to avoid the moon. You’ll have to find a way to work around it. Try observing in a shadow of a large structure (like a barn), or in a mountain shadow. Just try to keep the moon out of view. Let your eyes adjust to the darkness for a period, say, 15 minutes to half an hour. Just wait and watch, don’t expect too much, and see what you see.

Visit Sunrise Sunset Calendars and check the astronomical twilight and moonrise and moonset boxes to learn these key elements.

12 small objects streaking toward Earth viewed from orbit in black and white.

Leonid meteors, viewed from space in 1997. Image via NASA.

Where should you watch the meteor shower? We hear lots of reports from people who see meteors from yards, decks, streets and especially highways in and around cities. But the best place to watch a meteor shower is always in the country. Just go far enough from town that glittering stars, the same stars drowned by city lights, begin to pop into view.

Find a place to watch – or recommend a place – at EarthSky’s Best Places to Stargaze page.

City, state and national parks are often great places to watch meteor showers. Try Googling the name of your state or city with the words city park, state park or national park. Then, be sure to go to the park early in the day and find a wide open area with a good view of the sky in all directions.

When night falls, you’ll probably be impatient to see meteors. But remember that the shower is best after midnight. Catch a nap in early evening if you can. After midnight, lie back comfortably and watch as best you can in all parts of the sky.

Sometimes friends like to watch together, facing different directions. When somebody sees one, they can call out meteor! Then everyone can quickly turn to get a glimpse.

Star chart of constellation Leo with radial arrows at upper end.

Regulus, the brightest star in the constellation Leo the Lion, dots a backwards question mark of stars known as the Sickle. If you trace all the Leonid meteors backward, they appear to radiate from this area of the sky.

Which direction should I look to see the Leonids? Meteors in annual showers are named for the point in our sky from which they appear to radiate. This shower is named for the constellation Leo the Lion, because these meteors radiate outward from the vicinity of stars representing the Lion’s Mane.

If you trace the paths of Leonid meteors backward on the sky’s dome, they do seem to stream from near the star Algieba in the constellation Leo. The point in the sky from which they appear to radiate is called the radiant point. This radiant point is an optical illusion. It’s like standing on railroad tracks and peering off into the distance to see the tracks converge. The illusion of the radiant point is caused by the fact that the meteors – much like the railroad tracks – are moving on parallel paths.

In recent years, people have gotten the mistaken idea that you must know the whereabouts of a meteor shower’s radiant point in order to watch the meteor shower. You don’t need to. The meteors often don’t become visible until they are 30 degrees or so from their radiant point. They are streaking out from the radiant in all directions.

Thus the Leonid meteors – like meteors in all annual showers – will appear in all parts of the sky.

Etchings of meteors over Niagara Falls and a scene with people looking up at meteors.

Old woodcuts depicting 1833 Leonid meteor storm – “the night the stars fell.”

Will the Leonids produce a meteor storm in 2019? Let’s hope not! It would be so frustrating if a meteor storm took place with a bright moon in the sky. No Leonid meteor storm is expected in 2019, however. Most astronomers say you need more than 1,000 meteors an hour to consider a shower as a storm. That’s a far cry from the 10 to 15 meteors per hour predicted for the Leonids in most years (including this year if there were no moon in the sky).

Of course, seeing even one bright meteor can make your night.

The Leonid shower is known for producing meteor storms, though. The parent comet – Tempel-Tuttle – completes a single orbit around the sun about once every 33 years. It releases fresh material every time it enters the inner solar system and approaches the sun. Since the 19th century, skywatchers have watched for Leonid meteor storms about every 33 years, beginning with the meteor storm of 1833, said to produce more than 100,000 meteors an hour.

The next great Leonid storms were seen about 33 years later, in 1866 and 1867.

Then a meteor storm was predicted for 1899, but did not materialize.

It wasn’t until 1966 that the next spectacular Leonid storm was seen, this time over the Americas. In 1966, observers in the southwest United States reported seeing 40 to 50 meteors per second (that’s 2,400 to 3,000 meteors per minute!) during a span of 15 minutes on the morning of November 17, 1966.

In 2001, another great Leonid meteor storm occurred. Spaceweather.com reported:

The display began on Sunday morning, November 18, when Earth glided into a dust cloud shed by Comet Tempel-Tuttle in 1766. Thousands of meteors per hour rained over North America and Hawaii. Then, on Monday morning November 19 (local time in Asia), it happened again: Earth entered a second cometary debris cloud from Tempel-Tuttle. Thousands more Leonids then fell over east Asian countries and Australia.

View SpaceWeather’s 2001 Leonid meteor gallery.

Bottom line: If you want to watch the 2019 Leonid meteor shower, just know that the hours between midnight and dawn are best for meteor-watching. Unfortunately, this year, a waning gibbous moon will drown all but the brightest meteors from the sky. Still, if you look, you might see some!

EarthSky’s meteor shower guide for 2019

Enjoying EarthSky? Sign up for our free daily newsletter today!

Easily locate stars and constellations during any day and time with EarthSky’s Planisphere.



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Round overexposed moon and long thin white streak.

This isn’t a Leonid meteor. It’s an Orionid. But – as this photo shows – you can sometimes catch a meteor in bright moonlight, assuming it’s bright enough. Photo taken in late October 2016 by Eliot Herman in Tucson, Arizona. Thanks, Eliot!

November’s wonderful Leonid meteor shower is active from about November 6 to 30 each year. The peak is expected in 2019 on the night of November 17 (morning of November 18). The shower happens as our world crosses the orbital path of Comet 55P/Tempel-Tuttle. Like many comets, Tempel-Tuttle litters its orbit with bits of debris. It’s when this cometary debris enters Earth’s atmosphere and vaporizes that we see the Leonid meteor shower. In 2019, a waning gibbous moon will light up the sky during the shower’s peak. In a dark sky, absent of moonlight, you can see up to 10 to 15 meteors per hour at the peak. In 2019’s moonlit sky? We can’t predict, but some of the brighter meteors should be visible in moonlight.

Although this shower is known for its periodic storms, no Leonid storm is expected this year. Keep reading to learn more.

The 2019 lunar calendars are here! Order yours before they’re gone. Makes a great gift.

Thin white almost vertical streak over dark, distant hilly horizon.

James Younger sent in this photo during the 2015 peak of the Leonid meteor shower. It’s a meteor over the San Juan Islands in the Pacific Northwest, between the U.S. mainland and Vancouver Island, British Columbia.

How many Leonid meteors will you see in 2019? The answer always depends on when you watch, where you watch, and on the clarity and darkness of your night sky.

In 2019, no matter where you are on Earth – and no matter when you watch, on the morning of the peak itself, or on the morning leading up to the peak – the best hours of the night for meteor-watching will be hindered by the bright moon. Those hours are between midnight and dawn, when Earth’s forward motion through space has carried your part of Earth head-on into the meteor stream.

Also in 2019, there’s really no way to avoid the moon. You’ll have to find a way to work around it. Try observing in a shadow of a large structure (like a barn), or in a mountain shadow. Just try to keep the moon out of view. Let your eyes adjust to the darkness for a period, say, 15 minutes to half an hour. Just wait and watch, don’t expect too much, and see what you see.

Visit Sunrise Sunset Calendars and check the astronomical twilight and moonrise and moonset boxes to learn these key elements.

12 small objects streaking toward Earth viewed from orbit in black and white.

Leonid meteors, viewed from space in 1997. Image via NASA.

Where should you watch the meteor shower? We hear lots of reports from people who see meteors from yards, decks, streets and especially highways in and around cities. But the best place to watch a meteor shower is always in the country. Just go far enough from town that glittering stars, the same stars drowned by city lights, begin to pop into view.

Find a place to watch – or recommend a place – at EarthSky’s Best Places to Stargaze page.

City, state and national parks are often great places to watch meteor showers. Try Googling the name of your state or city with the words city park, state park or national park. Then, be sure to go to the park early in the day and find a wide open area with a good view of the sky in all directions.

When night falls, you’ll probably be impatient to see meteors. But remember that the shower is best after midnight. Catch a nap in early evening if you can. After midnight, lie back comfortably and watch as best you can in all parts of the sky.

Sometimes friends like to watch together, facing different directions. When somebody sees one, they can call out meteor! Then everyone can quickly turn to get a glimpse.

Star chart of constellation Leo with radial arrows at upper end.

Regulus, the brightest star in the constellation Leo the Lion, dots a backwards question mark of stars known as the Sickle. If you trace all the Leonid meteors backward, they appear to radiate from this area of the sky.

Which direction should I look to see the Leonids? Meteors in annual showers are named for the point in our sky from which they appear to radiate. This shower is named for the constellation Leo the Lion, because these meteors radiate outward from the vicinity of stars representing the Lion’s Mane.

If you trace the paths of Leonid meteors backward on the sky’s dome, they do seem to stream from near the star Algieba in the constellation Leo. The point in the sky from which they appear to radiate is called the radiant point. This radiant point is an optical illusion. It’s like standing on railroad tracks and peering off into the distance to see the tracks converge. The illusion of the radiant point is caused by the fact that the meteors – much like the railroad tracks – are moving on parallel paths.

In recent years, people have gotten the mistaken idea that you must know the whereabouts of a meteor shower’s radiant point in order to watch the meteor shower. You don’t need to. The meteors often don’t become visible until they are 30 degrees or so from their radiant point. They are streaking out from the radiant in all directions.

Thus the Leonid meteors – like meteors in all annual showers – will appear in all parts of the sky.

Etchings of meteors over Niagara Falls and a scene with people looking up at meteors.

Old woodcuts depicting 1833 Leonid meteor storm – “the night the stars fell.”

Will the Leonids produce a meteor storm in 2019? Let’s hope not! It would be so frustrating if a meteor storm took place with a bright moon in the sky. No Leonid meteor storm is expected in 2019, however. Most astronomers say you need more than 1,000 meteors an hour to consider a shower as a storm. That’s a far cry from the 10 to 15 meteors per hour predicted for the Leonids in most years (including this year if there were no moon in the sky).

Of course, seeing even one bright meteor can make your night.

The Leonid shower is known for producing meteor storms, though. The parent comet – Tempel-Tuttle – completes a single orbit around the sun about once every 33 years. It releases fresh material every time it enters the inner solar system and approaches the sun. Since the 19th century, skywatchers have watched for Leonid meteor storms about every 33 years, beginning with the meteor storm of 1833, said to produce more than 100,000 meteors an hour.

The next great Leonid storms were seen about 33 years later, in 1866 and 1867.

Then a meteor storm was predicted for 1899, but did not materialize.

It wasn’t until 1966 that the next spectacular Leonid storm was seen, this time over the Americas. In 1966, observers in the southwest United States reported seeing 40 to 50 meteors per second (that’s 2,400 to 3,000 meteors per minute!) during a span of 15 minutes on the morning of November 17, 1966.

In 2001, another great Leonid meteor storm occurred. Spaceweather.com reported:

The display began on Sunday morning, November 18, when Earth glided into a dust cloud shed by Comet Tempel-Tuttle in 1766. Thousands of meteors per hour rained over North America and Hawaii. Then, on Monday morning November 19 (local time in Asia), it happened again: Earth entered a second cometary debris cloud from Tempel-Tuttle. Thousands more Leonids then fell over east Asian countries and Australia.

View SpaceWeather’s 2001 Leonid meteor gallery.

Bottom line: If you want to watch the 2019 Leonid meteor shower, just know that the hours between midnight and dawn are best for meteor-watching. Unfortunately, this year, a waning gibbous moon will drown all but the brightest meteors from the sky. Still, if you look, you might see some!

EarthSky’s meteor shower guide for 2019

Enjoying EarthSky? Sign up for our free daily newsletter today!

Easily locate stars and constellations during any day and time with EarthSky’s Planisphere.



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Colorado moon



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Watch spacewalk on Friday November 15

View of Earth beyond large, complex, mostly gleaming white components of ISS, one marked AMS.

This picture, taken during a July 2011 spacewalk, shows the International Space Station with space shuttle Atlantis (docked at the edge of the frame on the far right) and a Russian Soyuz spacecraft (docked below the sun). In the foreground is the Alpha Magnetic Spectrometer (AMS) experiment, which will be repaired by astronauts in upcoming spacewalks, the first of which is November 15, 2019. Image via NASA/Ron Garan.

On Friday, November 15, 2019, two astronauts will venture outside the International Space Station for the first of a series of complex spacewalks to repair a cosmic ray detector.

NASA TV begins its live spacewalk coverage Friday at 10:30 UTC (5:30 a.m. EST). Translate UTC to your time. The astronauts, Luca Parmitano of ESA (European Space Agency) and NASA Flight Engineer Drew Morgan will set their spacesuits to battery power at 12:05 UTC (7:05 a.m EST), signifying the start of their spacewalk.

Friday’s spacewalk will be the first of at least four spacewalks currently planned before the end of this year (the others are as yet unscheduled) to repair the Alpha Magnetic Spectrometer (AMS), a cosmic ray detector.

Over the course of the spacewalks, the astronauts will replace a cooling system and fix a coolant leak on AMS. Delivered to the station in May 2011, AMS captures cosmic particles and measures their electrical charge in its search for antimatter and dark matter. The upgraded cooling system will support AMS through the lifetime of the space station.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Three astronauts in blue shirts in small round chamber with three windows visible.

Astronauts (from left) Luca Parmitano, Christina Koch and Andrew Morgan are pictured at the robotics workstation inside the cupola, the International Space Station’s “window to the world.” Image via NASA.

According to a NASA statement:

These spacewalks are considered the most complex of their kind since the Hubble Space Telescope servicing missions, which took place between 1993 and 2009. The AMS originally was designed for a three-year mission and, unlike Hubble, was not designed to be serviced once in space. More than 20 unique tools were designed for the intricate repair work, which will include the cutting and splicing of eight cooling tubes to be connected to the new system, and reconnection of a myriad of power and data cables. Astronauts have never cut and reconnected fluid lines during a spacewalk.

Parmitano and Morgan have spent dozens of hours training specifically for the AMS repair spacewalks. NASA astronauts Christina Koch and Jessica Meir will support the duo on Friday. Meir will be in charge of the Canadarm2 robotic arm while Koch manages the U.S. spacesuits.

Bottom line: Watch ISS astronauts spacewalk live on November 15, 2019.

Via NASA



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View of Earth beyond large, complex, mostly gleaming white components of ISS, one marked AMS.

This picture, taken during a July 2011 spacewalk, shows the International Space Station with space shuttle Atlantis (docked at the edge of the frame on the far right) and a Russian Soyuz spacecraft (docked below the sun). In the foreground is the Alpha Magnetic Spectrometer (AMS) experiment, which will be repaired by astronauts in upcoming spacewalks, the first of which is November 15, 2019. Image via NASA/Ron Garan.

On Friday, November 15, 2019, two astronauts will venture outside the International Space Station for the first of a series of complex spacewalks to repair a cosmic ray detector.

NASA TV begins its live spacewalk coverage Friday at 10:30 UTC (5:30 a.m. EST). Translate UTC to your time. The astronauts, Luca Parmitano of ESA (European Space Agency) and NASA Flight Engineer Drew Morgan will set their spacesuits to battery power at 12:05 UTC (7:05 a.m EST), signifying the start of their spacewalk.

Friday’s spacewalk will be the first of at least four spacewalks currently planned before the end of this year (the others are as yet unscheduled) to repair the Alpha Magnetic Spectrometer (AMS), a cosmic ray detector.

Over the course of the spacewalks, the astronauts will replace a cooling system and fix a coolant leak on AMS. Delivered to the station in May 2011, AMS captures cosmic particles and measures their electrical charge in its search for antimatter and dark matter. The upgraded cooling system will support AMS through the lifetime of the space station.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Three astronauts in blue shirts in small round chamber with three windows visible.

Astronauts (from left) Luca Parmitano, Christina Koch and Andrew Morgan are pictured at the robotics workstation inside the cupola, the International Space Station’s “window to the world.” Image via NASA.

According to a NASA statement:

These spacewalks are considered the most complex of their kind since the Hubble Space Telescope servicing missions, which took place between 1993 and 2009. The AMS originally was designed for a three-year mission and, unlike Hubble, was not designed to be serviced once in space. More than 20 unique tools were designed for the intricate repair work, which will include the cutting and splicing of eight cooling tubes to be connected to the new system, and reconnection of a myriad of power and data cables. Astronauts have never cut and reconnected fluid lines during a spacewalk.

Parmitano and Morgan have spent dozens of hours training specifically for the AMS repair spacewalks. NASA astronauts Christina Koch and Jessica Meir will support the duo on Friday. Meir will be in charge of the Canadarm2 robotic arm while Koch manages the U.S. spacesuits.

Bottom line: Watch ISS astronauts spacewalk live on November 15, 2019.

Via NASA



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All you need to know: The famous Orion Nebula

Hazy view of constellation Orion in sky over small rectangular house.

View larger. | Stefan Nilsson captured this image in southern Sweden in 2017. You can recognize the constellation Orion by his 3 Belt stars, three stars in a short, straight row. The Orion Nebula is that red fuzzy region in Orion’s Sword, hanging from the Belt.

Many people are familiar with Orion, the most noticeable of all constellations. The three stars of Orion’s Belt jump out at you midway between Orion’s two brightest stars, Betelgeuse and Rigel. Once you find the Belt stars, you can also locate the Orion Nebula, otherwise known as M42, a stellar nursery where new stars are being born.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Star field with three bright stars in a row and a small but distinct pink nebula below.

View larger. | The three medium-bright stars in a short, straight row represent Orion’s Belt. A curved line of stars extending from the Belt represents Orion’s Sword. The Orion Nebula lies about midway down in the Sword of Orion. Image via Marian McGaffney.

Pink and blue nebula with small circle over big hemicircle fills image.

Orion Nebula captured on February 5, 2016, by Scott MacNeill at Frosty Drew Observatory in Charlestown, Rhode Island. Scott said this image is a composite of 25 shots.

How to locate the Orion Nebula. If you want to find this famous nebula, first you have to locate the constellation Orion. Fortunately, that’s easy, if you’re looking at the right time of year. The Northern Hemisphere winter months (Southern Hemisphere summer months) are the perfect time to come to know Orion.

The constellation is noticeable for three medium-bright stars in a short, straight row. These stars represent Orion’s Belt.

If you look closely, you’ll notice a curved line of stars “hanging” from the three Belt stars. These stars represent Orion’s Sword. Look for the Orion Nebula about midway down in the Sword of Orion.

As a general rule, the higher the constellation Orion is in the sky, the easier it is to see the Orion Nebula. From Northern Hemisphere locations, Orion is due south and highest in the sky around midnight in middle December. The stars return to the same place in the sky some four minutes earlier each night, or two hours earlier each month. So look for Orion to be highest up around 10 p.m. in mid-January and 8 p.m. in mid-February.

Another time people notice Orion is around the months of August and September, when this constellation appears in the east before dawn.

Most nebulae – clouds of interstellar gas and dust – are difficult if not impossible to see with the unaided eye or even binoculars. But the Orion Nebula is in a class nearly all by itself. It’s visible to the unaided eye on a dark, moonless night. To me, it looks like a star encased in a globe of luminescent fog. The dark-sky aficionado Stephen James O’Meara described it as:

… angel’s breath against a frosted sky.

In a dark country sky, observe the Orion Nebula for yourself to see what it looks like. A backyard telescope, or even binoculars, do wonders to showcase one of the greatest celestial treasures in the winter sky.

Swirled, stretched multicolor clouds in star field.

This spectacular image of the Orion Nebula star-formation region was obtained from multiple exposures using the HAWK-I infrared camera on ESO’s Very Large Telescope in Chile. Image via ESO/H. Drass et al.

Detailed many-colored nebula with scattered stars.

The Orion Nebula, 1,500 light years from Earth. Image via NASA/JPL-Caltech/STScI.

What science says about the Orion Nebula. According to modern astronomers, the Orion Nebula is an enormous cloud of gas and dust, one of many in our Milky Way galaxy. It lies roughly 1,300 light-years from Earth.

At some 30 to 40 light-years in diameter, this great big nebulous cocoon is giving birth to perhaps a thousand stars. A young open star cluster, whose stars were born at the same time from a portion of the nebula and are still loosely bound by gravity, can be seen within the nebula. It is sometimes called the Orion Nebula Star Cluster. In 2012, an international team of astronomers suggested this cluster in the Orion Nebula might have a black hole at its heart.

The four brightest stars in the Orion Nebula can be seen through amateur astronomers’ telescopes and are affectionately known as The Trapezium. The light of the young, hot Trapezium stars illuminate the Orion Nebula. These stars are only a million or so years old – babies on the scale of star lifetimes.

But most of the stars in this emerging cluster are veiled behind the Orion Nebula itself, the great stellar nursery in Orion’s Sword.

Orion Nebula’s position is Right Ascension: 5h 35.4m; Declination: 5o 27′ south

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Bottom line: To find the Orion Nebula in your night sky, look below Orion’s Belt. Your eye sees it as a tiny, hazy spot, but it’s a vast region of star formation.



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Hazy view of constellation Orion in sky over small rectangular house.

View larger. | Stefan Nilsson captured this image in southern Sweden in 2017. You can recognize the constellation Orion by his 3 Belt stars, three stars in a short, straight row. The Orion Nebula is that red fuzzy region in Orion’s Sword, hanging from the Belt.

Many people are familiar with Orion, the most noticeable of all constellations. The three stars of Orion’s Belt jump out at you midway between Orion’s two brightest stars, Betelgeuse and Rigel. Once you find the Belt stars, you can also locate the Orion Nebula, otherwise known as M42, a stellar nursery where new stars are being born.

EarthSky 2020 lunar calendars are available! They make great gifts. Order now. Going fast!

Star field with three bright stars in a row and a small but distinct pink nebula below.

View larger. | The three medium-bright stars in a short, straight row represent Orion’s Belt. A curved line of stars extending from the Belt represents Orion’s Sword. The Orion Nebula lies about midway down in the Sword of Orion. Image via Marian McGaffney.

Pink and blue nebula with small circle over big hemicircle fills image.

Orion Nebula captured on February 5, 2016, by Scott MacNeill at Frosty Drew Observatory in Charlestown, Rhode Island. Scott said this image is a composite of 25 shots.

How to locate the Orion Nebula. If you want to find this famous nebula, first you have to locate the constellation Orion. Fortunately, that’s easy, if you’re looking at the right time of year. The Northern Hemisphere winter months (Southern Hemisphere summer months) are the perfect time to come to know Orion.

The constellation is noticeable for three medium-bright stars in a short, straight row. These stars represent Orion’s Belt.

If you look closely, you’ll notice a curved line of stars “hanging” from the three Belt stars. These stars represent Orion’s Sword. Look for the Orion Nebula about midway down in the Sword of Orion.

As a general rule, the higher the constellation Orion is in the sky, the easier it is to see the Orion Nebula. From Northern Hemisphere locations, Orion is due south and highest in the sky around midnight in middle December. The stars return to the same place in the sky some four minutes earlier each night, or two hours earlier each month. So look for Orion to be highest up around 10 p.m. in mid-January and 8 p.m. in mid-February.

Another time people notice Orion is around the months of August and September, when this constellation appears in the east before dawn.

Most nebulae – clouds of interstellar gas and dust – are difficult if not impossible to see with the unaided eye or even binoculars. But the Orion Nebula is in a class nearly all by itself. It’s visible to the unaided eye on a dark, moonless night. To me, it looks like a star encased in a globe of luminescent fog. The dark-sky aficionado Stephen James O’Meara described it as:

… angel’s breath against a frosted sky.

In a dark country sky, observe the Orion Nebula for yourself to see what it looks like. A backyard telescope, or even binoculars, do wonders to showcase one of the greatest celestial treasures in the winter sky.

Swirled, stretched multicolor clouds in star field.

This spectacular image of the Orion Nebula star-formation region was obtained from multiple exposures using the HAWK-I infrared camera on ESO’s Very Large Telescope in Chile. Image via ESO/H. Drass et al.

Detailed many-colored nebula with scattered stars.

The Orion Nebula, 1,500 light years from Earth. Image via NASA/JPL-Caltech/STScI.

What science says about the Orion Nebula. According to modern astronomers, the Orion Nebula is an enormous cloud of gas and dust, one of many in our Milky Way galaxy. It lies roughly 1,300 light-years from Earth.

At some 30 to 40 light-years in diameter, this great big nebulous cocoon is giving birth to perhaps a thousand stars. A young open star cluster, whose stars were born at the same time from a portion of the nebula and are still loosely bound by gravity, can be seen within the nebula. It is sometimes called the Orion Nebula Star Cluster. In 2012, an international team of astronomers suggested this cluster in the Orion Nebula might have a black hole at its heart.

The four brightest stars in the Orion Nebula can be seen through amateur astronomers’ telescopes and are affectionately known as The Trapezium. The light of the young, hot Trapezium stars illuminate the Orion Nebula. These stars are only a million or so years old – babies on the scale of star lifetimes.

But most of the stars in this emerging cluster are veiled behind the Orion Nebula itself, the great stellar nursery in Orion’s Sword.

Orion Nebula’s position is Right Ascension: 5h 35.4m; Declination: 5o 27′ south

Enjoying EarthSky? Sign up for our free daily newsletter today!

Bottom line: To find the Orion Nebula in your night sky, look below Orion’s Belt. Your eye sees it as a tiny, hazy spot, but it’s a vast region of star formation.



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10 years 10 suns

Ten yellow circles on a black background

View larger. | The individual frames of the image shown here were captured on (top row, left to right): 20 February 20, 2010; February 1, 2011; January 20, 2012; February 5, 2013; January 28, 2014; and (bottom row, left to right) January 19, 2015; February 5, 2016; January 22, 2017; February 2, 2018: February 1, 2019. Image via ESA/Royal Observatory of Belgium.

Last week marked 10 years that ESA’s Proba-2 satellite (launched on November 2, 2009) has been orbiting the Earth, imaging and observing the sun.

This image, released by ESA on November 10, 2019, shows 10 different views of the sun captured throughout Proba-2’s lifetime, processed to highlight the extended solar atmosphere – the part of the atmosphere that’s visible around the sun’s main circular disc.

According to a statement from ESA about the image:

The sun’s activity has a cycle of about 11 years, with the presence and strength of phenomena such as flares, coronal mass ejections, dark ‘coronal holes’ and bright ‘active regions’ fluctuating accordingly. These images were taken by Proba-2’s extreme-ultraviolet SWAP instrument, and show a snapshot of the sun in January or February of each year from 2010 to 2019 (with the oldest frame on the top left, and the most recent to the bottom right). This mosaic thus neatly shows the variability in the solar atmosphere in beautiful detail, demonstrating how this cycle affects the sun. The sun begins in a phase of low activity (solar minimum: top left) in 2010; enters a phase of increasing activity and then shows highest activity in 2014 (solar maximum: top right). It slowly calms down again to enter a low-activity phase in 2019 (another minimum: bottom right).

Bottom line: Ten images of the sun taken by the ESA Proba-2 satellite, one from each year from 2010 to 2019.

Via ESA



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Ten yellow circles on a black background

View larger. | The individual frames of the image shown here were captured on (top row, left to right): 20 February 20, 2010; February 1, 2011; January 20, 2012; February 5, 2013; January 28, 2014; and (bottom row, left to right) January 19, 2015; February 5, 2016; January 22, 2017; February 2, 2018: February 1, 2019. Image via ESA/Royal Observatory of Belgium.

Last week marked 10 years that ESA’s Proba-2 satellite (launched on November 2, 2009) has been orbiting the Earth, imaging and observing the sun.

This image, released by ESA on November 10, 2019, shows 10 different views of the sun captured throughout Proba-2’s lifetime, processed to highlight the extended solar atmosphere – the part of the atmosphere that’s visible around the sun’s main circular disc.

According to a statement from ESA about the image:

The sun’s activity has a cycle of about 11 years, with the presence and strength of phenomena such as flares, coronal mass ejections, dark ‘coronal holes’ and bright ‘active regions’ fluctuating accordingly. These images were taken by Proba-2’s extreme-ultraviolet SWAP instrument, and show a snapshot of the sun in January or February of each year from 2010 to 2019 (with the oldest frame on the top left, and the most recent to the bottom right). This mosaic thus neatly shows the variability in the solar atmosphere in beautiful detail, demonstrating how this cycle affects the sun. The sun begins in a phase of low activity (solar minimum: top left) in 2010; enters a phase of increasing activity and then shows highest activity in 2014 (solar maximum: top right). It slowly calms down again to enter a low-activity phase in 2019 (another minimum: bottom right).

Bottom line: Ten images of the sun taken by the ESA Proba-2 satellite, one from each year from 2010 to 2019.

Via ESA



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Orion the Hunter now easy to view

Tonight, watch for Orion the Hunter – perhaps the easiest to identify of all constellations – rising at mid-evening. It’s around late November and early December that people begin to notice Orion in the evening sky, and to comment on it. Orion will climb over your eastern horizon by around 9 p.m. tonight. You can find this constellation and watch it for months to come.

The most noticeable part of Orion is the pattern called Orion’s Belt: three medium-bright stars in a short, straight row. As seen from mid-northern latitudes, Orion appears to be lying on his side – with his Belt stars pointing upward – when he first ascends into our eastern sky in mid-evening at this time of year. Orion’s two brightest stars – Betelgeuse and Rigel – shine on opposite sides of the Belt.

Stars trails of constellation Orion via EarthSky Facebook friend Jean Baptiste Feldman. Can you pick out the three stars in Orion’s Belt? Notice also the different colors of the stars in Orion.

As night passes, and Earth spins beneath the sky, Orion will climb higher in our sky. When this constellation is highest in the south, it is a huge, noticeable star pattern. But Orion doesn’t reach its highest point until an hour or two after midnight (that’s local time, for all times zones around the world) at this time of year.

Like all the stars, Orion’s stars rise some four minutes earlier with each passing day, or about two hours earlier with each passing month. If you see Orion shining in the east at 9 p.m. tonight, look for Orion to be in the same place in the sky at about 7 p.m. a month from now. Or if Orion is due south at 2 a.m. tomorrow, look for Orion to be due south at 12 midnight p.m. one month later.

Orion chart

This chart shows the famous constellation of Orion (The Hunter). From northerly latitudes in the Northern Hemisphere, Orion stands upright in the southern sky (as pictured above) when this constellation reaches its highest point for the night. From temperate latitudes in the Southern Hemisphere, however, Orion is seen “upside-down” in the northern sky when the Hunter reaches its highest point for the night.

This shift in Orion’s location is due to Earth’s movement in orbit around the sun. As we move around the sun, our perspective on the stars surrounding us shifts. At the same hour daily, all the stars in the eastern half of the sky climb up a bit higher, whereas all the stars in the western half of the sky sink a bit closer to the western horizon.

Mirror view of Orion the Hunter from Johannes Hevelius' Uranographia (1690).

Are you familiar with the W- or M-shaped constellation Cassiopeia the Queen? Or Polaris, the North Star? As Orion rises in the east this evening, look for Cassiopeia to soar to her highest point for the night, above Polaris in the northern sky.

Karthik Easvur caught the constellation Orion on November 26, 2016, from his balcony in Hyderabad, India. The round translucent object in the photo, by the way, is a lens flare - an internal reflection from Karthik's camera - like caused by the same artificial light that's illuminating the palm tree on the right.

Karthik Easvur caught the constellation Orion on November 26, 2016, from his balcony in Hyderabad, India. The round translucent object in the photo, by the way, is a lens flare – an internal reflection from Karthik’s camera – likely caused by the same artificial light that’s illuminating the palm tree on the right.

Bottom line: By mid-to-late November, the famous constellation Orion the Hunter is back in the evening sky! Its most recognizable feature is a short, straight line of three medium-bright stars.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

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Tonight, watch for Orion the Hunter – perhaps the easiest to identify of all constellations – rising at mid-evening. It’s around late November and early December that people begin to notice Orion in the evening sky, and to comment on it. Orion will climb over your eastern horizon by around 9 p.m. tonight. You can find this constellation and watch it for months to come.

The most noticeable part of Orion is the pattern called Orion’s Belt: three medium-bright stars in a short, straight row. As seen from mid-northern latitudes, Orion appears to be lying on his side – with his Belt stars pointing upward – when he first ascends into our eastern sky in mid-evening at this time of year. Orion’s two brightest stars – Betelgeuse and Rigel – shine on opposite sides of the Belt.

Stars trails of constellation Orion via EarthSky Facebook friend Jean Baptiste Feldman. Can you pick out the three stars in Orion’s Belt? Notice also the different colors of the stars in Orion.

As night passes, and Earth spins beneath the sky, Orion will climb higher in our sky. When this constellation is highest in the south, it is a huge, noticeable star pattern. But Orion doesn’t reach its highest point until an hour or two after midnight (that’s local time, for all times zones around the world) at this time of year.

Like all the stars, Orion’s stars rise some four minutes earlier with each passing day, or about two hours earlier with each passing month. If you see Orion shining in the east at 9 p.m. tonight, look for Orion to be in the same place in the sky at about 7 p.m. a month from now. Or if Orion is due south at 2 a.m. tomorrow, look for Orion to be due south at 12 midnight p.m. one month later.

Orion chart

This chart shows the famous constellation of Orion (The Hunter). From northerly latitudes in the Northern Hemisphere, Orion stands upright in the southern sky (as pictured above) when this constellation reaches its highest point for the night. From temperate latitudes in the Southern Hemisphere, however, Orion is seen “upside-down” in the northern sky when the Hunter reaches its highest point for the night.

This shift in Orion’s location is due to Earth’s movement in orbit around the sun. As we move around the sun, our perspective on the stars surrounding us shifts. At the same hour daily, all the stars in the eastern half of the sky climb up a bit higher, whereas all the stars in the western half of the sky sink a bit closer to the western horizon.

Mirror view of Orion the Hunter from Johannes Hevelius' Uranographia (1690).

Are you familiar with the W- or M-shaped constellation Cassiopeia the Queen? Or Polaris, the North Star? As Orion rises in the east this evening, look for Cassiopeia to soar to her highest point for the night, above Polaris in the northern sky.

Karthik Easvur caught the constellation Orion on November 26, 2016, from his balcony in Hyderabad, India. The round translucent object in the photo, by the way, is a lens flare - an internal reflection from Karthik's camera - like caused by the same artificial light that's illuminating the palm tree on the right.

Karthik Easvur caught the constellation Orion on November 26, 2016, from his balcony in Hyderabad, India. The round translucent object in the photo, by the way, is a lens flare – an internal reflection from Karthik’s camera – likely caused by the same artificial light that’s illuminating the palm tree on the right.

Bottom line: By mid-to-late November, the famous constellation Orion the Hunter is back in the evening sky! Its most recognizable feature is a short, straight line of three medium-bright stars.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky https://ift.tt/2DKFoYT

Ultima Thule renamed to avoid Nazi link

Ultima Thule looks like 2 snowballs stuck together. It is pockmarked with craters.

Here’s the object formerly known as 2014 MU69 – then briefly as Ultima Thule – and now as Arrokoth. It’s roughly 19 miles (30 km) long, or about 1/60th the diameter of Pluto. Image via NASA/ Johns Hopkins University Applied Physics Laboratory/ Southwest Research Institute/ Spaceflight Insider.

Darn. Like many others, I had really liked the name Ultima Thule for an object on the fringes of our solar system, the most distant object ever to be visited by an earthly spacecraft. The name is a mythological reference to a faraway, mysterious land, someplace distant and cold. The craft that visited it was, of course, New Horizons, same craft that gave us the amazing images of Pluto in 2015. Following its Pluto encounter, New Horizons was pushing on into the Kuiper Belt, aiming toward an object known originally as 2014 MU69, when space scientists and the public decided it needed a new name. Shortly before the New Horizons encounter on January 1, 2019, they chose the name to Ultima Thule. Then a reporter at Newsweek pointed out that the Nazi party had used the phrase Ultima Thule to refer to the mythical homeland of the Aryan people. The term apparently remains in use by modern so-called alt-right groups. Now the object has a new name yet again. The name is now Arrokoth, which means sky in the Powhatan and Algonquian languages.

NASA held a naming ceremony to give 2014 MU69 its new official name Arrokoth yesterday (November 12, 2019). The name was chosen based on the local Native American culture in Maryland, where the New Horizons mission control center is based.

A wealth of data from New Horizons’ encounter with Arrokoth is still being sent back from the spacecraft to Earth for analysis. Scientists did use New HOrizons’ cameras to glimpse its strange, double-lobed shape, indicating a possible gentle collision of two objects long ago. Arrokoth also appears to be covered in methane or nitrogen ice, giving it a red tinge.

Toward the end of 2019, around the time the name Ultima Thule came into use, Mark Showalter, a planetary astronomer at the SETI Institute and investigator on the New Horizons mission who led the naming process, had told Newsweek:

‘Beyond the limits of the known world’—that’s such a beautiful metaphor for what we’re doing this year.

But the association with Nazis and the alt-right apparently caused “push-back.” Hence the name change. I just read a wonderful book on the alt-rights use of social media (Antisocial: Online Extremists, Techno-Utopians, and the Hijacking of the American Conversation, by Andrew Marantz). It it, he describes how the alt-right and white nationalist movements reject much of what mainstream media has to say as “lies.”

I can only imagine the mini-push-back going on in the alt-right media community today, given this name change.

Book cover of Antisocial

If you’re interested at all in the alt-right and white nationalist movement in the U.S., Antisocial by Andrew Marantz – a writer for the New Yorker – is an excellent, mind-opening and very readable book. Here’s its page on Amazon.

Bottom line: The Kuiper Belt object formerly known as 2014 MU69 – later known as Ultima Thule – has been renamed again. Its new name is Arrokoth.



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Ultima Thule looks like 2 snowballs stuck together. It is pockmarked with craters.

Here’s the object formerly known as 2014 MU69 – then briefly as Ultima Thule – and now as Arrokoth. It’s roughly 19 miles (30 km) long, or about 1/60th the diameter of Pluto. Image via NASA/ Johns Hopkins University Applied Physics Laboratory/ Southwest Research Institute/ Spaceflight Insider.

Darn. Like many others, I had really liked the name Ultima Thule for an object on the fringes of our solar system, the most distant object ever to be visited by an earthly spacecraft. The name is a mythological reference to a faraway, mysterious land, someplace distant and cold. The craft that visited it was, of course, New Horizons, same craft that gave us the amazing images of Pluto in 2015. Following its Pluto encounter, New Horizons was pushing on into the Kuiper Belt, aiming toward an object known originally as 2014 MU69, when space scientists and the public decided it needed a new name. Shortly before the New Horizons encounter on January 1, 2019, they chose the name to Ultima Thule. Then a reporter at Newsweek pointed out that the Nazi party had used the phrase Ultima Thule to refer to the mythical homeland of the Aryan people. The term apparently remains in use by modern so-called alt-right groups. Now the object has a new name yet again. The name is now Arrokoth, which means sky in the Powhatan and Algonquian languages.

NASA held a naming ceremony to give 2014 MU69 its new official name Arrokoth yesterday (November 12, 2019). The name was chosen based on the local Native American culture in Maryland, where the New Horizons mission control center is based.

A wealth of data from New Horizons’ encounter with Arrokoth is still being sent back from the spacecraft to Earth for analysis. Scientists did use New HOrizons’ cameras to glimpse its strange, double-lobed shape, indicating a possible gentle collision of two objects long ago. Arrokoth also appears to be covered in methane or nitrogen ice, giving it a red tinge.

Toward the end of 2019, around the time the name Ultima Thule came into use, Mark Showalter, a planetary astronomer at the SETI Institute and investigator on the New Horizons mission who led the naming process, had told Newsweek:

‘Beyond the limits of the known world’—that’s such a beautiful metaphor for what we’re doing this year.

But the association with Nazis and the alt-right apparently caused “push-back.” Hence the name change. I just read a wonderful book on the alt-rights use of social media (Antisocial: Online Extremists, Techno-Utopians, and the Hijacking of the American Conversation, by Andrew Marantz). It it, he describes how the alt-right and white nationalist movements reject much of what mainstream media has to say as “lies.”

I can only imagine the mini-push-back going on in the alt-right media community today, given this name change.

Book cover of Antisocial

If you’re interested at all in the alt-right and white nationalist movement in the U.S., Antisocial by Andrew Marantz – a writer for the New Yorker – is an excellent, mind-opening and very readable book. Here’s its page on Amazon.

Bottom line: The Kuiper Belt object formerly known as 2014 MU69 – later known as Ultima Thule – has been renamed again. Its new name is Arrokoth.



from EarthSky https://ift.tt/2pgAkpF