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Moon and Uranus in Pisces September 8

Tonight – September 8, 2017 – the waning gibbous moon and Uranus, the seventh planet outward from the sun, are near each other on the sky’s dome, in front of the constellation Pisces the Fishes. Although Uranus will remain within Pisces’ borders for the rest of this year, the moon will leave Pisces after a day or two. Around the world, the moon and Uranus will rise over the eastern horizon by around mid-evening, though you can find out a more specific time from an astronomical almanac.

With the moon so bright and so close to Uranus on the sky’s dome, you’re not likely to glimpse Uranus with the unaided eye. But keep reading. We give you an idea of its location, and links to detailed charts, in this post.

View larger. | José Luis Ruiz Gómez in Almería, Spain captured Uranus near the moon on January 15, 2016. He wrote:

View larger. | José Luis Ruiz Gómez in Almería, Spain captured Uranus near the moon on January 15, 2016. He wrote: “Why not try?”

Uranus was the first planet to be discovered by the telescope, by William Hershel on March 13, 1781. At a distance of about 19 astronomical units from Earth at present, this world is pretty easy to see through binoculars – if you know exactly where to look.

People with good vision – and good charts (scroll to bottom of page) – can see Uranus with the unaided eye on dark, moonless nights.

In your quest to locate Uranus, first make friends with the constellation Pisces after the moon leaves the evening sky, starting in a few more days. Familiar with the Great Square of Pegasus? If so, jump off from there to the constellation Pisces the Fishes. Then with a good sky chart and binoculars you just might catch Uranus, the seventh planet from the sun.

First find the signpost known as the Great Square of Pegasus. That’s your jumping off spot for finding Pisces’ place in the great celestial sea. Click here for a larger chart.

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

Bottom line: The moon and the planet Uranus both reside in front of the constellation Pisces the Fishes on September 8, 2017.



from EarthSky http://ift.tt/2gMQEWU

Tonight – September 8, 2017 – the waning gibbous moon and Uranus, the seventh planet outward from the sun, are near each other on the sky’s dome, in front of the constellation Pisces the Fishes. Although Uranus will remain within Pisces’ borders for the rest of this year, the moon will leave Pisces after a day or two. Around the world, the moon and Uranus will rise over the eastern horizon by around mid-evening, though you can find out a more specific time from an astronomical almanac.

With the moon so bright and so close to Uranus on the sky’s dome, you’re not likely to glimpse Uranus with the unaided eye. But keep reading. We give you an idea of its location, and links to detailed charts, in this post.

View larger. | José Luis Ruiz Gómez in Almería, Spain captured Uranus near the moon on January 15, 2016. He wrote:

View larger. | José Luis Ruiz Gómez in Almería, Spain captured Uranus near the moon on January 15, 2016. He wrote: “Why not try?”

Uranus was the first planet to be discovered by the telescope, by William Hershel on March 13, 1781. At a distance of about 19 astronomical units from Earth at present, this world is pretty easy to see through binoculars – if you know exactly where to look.

People with good vision – and good charts (scroll to bottom of page) – can see Uranus with the unaided eye on dark, moonless nights.

In your quest to locate Uranus, first make friends with the constellation Pisces after the moon leaves the evening sky, starting in a few more days. Familiar with the Great Square of Pegasus? If so, jump off from there to the constellation Pisces the Fishes. Then with a good sky chart and binoculars you just might catch Uranus, the seventh planet from the sun.

First find the signpost known as the Great Square of Pegasus. That’s your jumping off spot for finding Pisces’ place in the great celestial sea. Click here for a larger chart.

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

Bottom line: The moon and the planet Uranus both reside in front of the constellation Pisces the Fishes on September 8, 2017.



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Digital Classroom: Making the (Login) Connection

Updated! What you need to know about logging in at Science Buddies with Google Classroom.

from Science Buddies Blog http://ift.tt/2j9JHUc
Updated! What you need to know about logging in at Science Buddies with Google Classroom.

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Stream Critters Reveal Much About Water Quality

by Micka Peck

I was never a huge ‘bug person’ as a kid. It wasn’t that I bolted in terror at the sight of anything crawling my direction, but I didn’t greet a dangling spider with much enthusiasm either. My little brother, on the other hand, loved running through fields of tall grass in search of massive grasshoppers and butterflies. So, it may have come as a surprise to my family when a colleague and I eagerly set off to West Virginia in search of benthic macroinvertebrates, or the bottom-dwelling stream critters that lack backbones and are visible to the naked eye. Think insects, crayfish, worms, mussels, etc.

A couple of things piqued my interest about these creatures. I had learned that benthic macroinvertebrates are a crucial indicator for understanding water quality. While a single “grab sample” from a stream can tell you something about its water quality at that moment, macroinvertebrates are exposed to a range of conditions throughout their life stages in water. Therefore, they more accurately represent long-term conditions of water quality. Some macroinvertebrates are very sensitive to pollutants and as the water quality worsens, are less prevalent. All of our Region 3 states rely on macroinvertebrates to assess whether a waterbody is supporting aquatic life, so I thought I should go see what all the fuss was about.

We arrived at the stream bank in waders toting buckets, scrub brushes, and a large net. After surveying the stream, we chose a few spots with fast moving water and a variety of rocks and cobble, which are popular habitats due to their shelter from predators. With the net placed on the streambed facing upstream, I grabbed the scrub brush, brushed the rocks and let any attached macroinvertebrates float into the net. Next, I kicked the rocks in front of the net to stir up any macroinvertebrates hiding underneath and let the water guide them into the net. At times, it looked like I was dancing the twist in the middle of the stream. Then, I dumped the contents in the net into a bucket and marveled at the bounty. It was teeming with crayfish, scuds, larvae of mayflies, stoneflies, dragonflies, and so much more. And now, rather than feeling ambivalent, I’m filled with a sense of childish wonder at the many surprises a stream may hold.

Stay tuned for Part 2 – in the lab!

 

About the Author: Micka Peck is a physical scientist in EPA’s Mid-Atlantic Region working on improving impaired waters through total maximum daily loads (TMDLs), or water quality improvement plans.

 



from The EPA Blog http://ift.tt/2gKH3zR

by Micka Peck

I was never a huge ‘bug person’ as a kid. It wasn’t that I bolted in terror at the sight of anything crawling my direction, but I didn’t greet a dangling spider with much enthusiasm either. My little brother, on the other hand, loved running through fields of tall grass in search of massive grasshoppers and butterflies. So, it may have come as a surprise to my family when a colleague and I eagerly set off to West Virginia in search of benthic macroinvertebrates, or the bottom-dwelling stream critters that lack backbones and are visible to the naked eye. Think insects, crayfish, worms, mussels, etc.

A couple of things piqued my interest about these creatures. I had learned that benthic macroinvertebrates are a crucial indicator for understanding water quality. While a single “grab sample” from a stream can tell you something about its water quality at that moment, macroinvertebrates are exposed to a range of conditions throughout their life stages in water. Therefore, they more accurately represent long-term conditions of water quality. Some macroinvertebrates are very sensitive to pollutants and as the water quality worsens, are less prevalent. All of our Region 3 states rely on macroinvertebrates to assess whether a waterbody is supporting aquatic life, so I thought I should go see what all the fuss was about.

We arrived at the stream bank in waders toting buckets, scrub brushes, and a large net. After surveying the stream, we chose a few spots with fast moving water and a variety of rocks and cobble, which are popular habitats due to their shelter from predators. With the net placed on the streambed facing upstream, I grabbed the scrub brush, brushed the rocks and let any attached macroinvertebrates float into the net. Next, I kicked the rocks in front of the net to stir up any macroinvertebrates hiding underneath and let the water guide them into the net. At times, it looked like I was dancing the twist in the middle of the stream. Then, I dumped the contents in the net into a bucket and marveled at the bounty. It was teeming with crayfish, scuds, larvae of mayflies, stoneflies, dragonflies, and so much more. And now, rather than feeling ambivalent, I’m filled with a sense of childish wonder at the many surprises a stream may hold.

Stay tuned for Part 2 – in the lab!

 

About the Author: Micka Peck is a physical scientist in EPA’s Mid-Atlantic Region working on improving impaired waters through total maximum daily loads (TMDLs), or water quality improvement plans.

 



from The EPA Blog http://ift.tt/2gKH3zR

Marines Launch Affordable, Portable 3-D Printed Drone

This DIY drone project is opening new doors in battlefield surveillance for the Marine Corps.

from http://ift.tt/2eJQe2Q
This DIY drone project is opening new doors in battlefield surveillance for the Marine Corps.

from http://ift.tt/2eJQe2Q

Giant sunspots, solar flares, aurora alert!

Extreme UV flash from the powerful X9.3-class solar flare on September 6. Spaceweather.com called it “a decade-class flare.” Image via NASA SDO.

Sure, we’re headed toward solar minimum, but that didn’t keep the sun from acting up this week. Since last weekend, two gigantic sunspots – AR2673 and its pal AR2674 – have been seen from around the world by those using safe solar filters. They’ve been seen even with the (safely filtered) eye alone, making their way across the sun’s face. These Active Regions on the sun spawned multiple moderate (M-class) flares on September 4 and 5. Then yesterday – on September 6, 2017 – sunspot AR2673 erupted in a powerful X9.3-class solar flare, the strongest solar flare in more than a decade. Spaceweather.com reported the X-rays and UV radiation from the blast ionized the top of Earth’s atmosphere, causing a strong shortwave radio blackout over Europe, Africa and the Atlantic Ocean.

In the process of emitting the flares, AR2673 also blasted a coronal mass ejection (CME) into space in Earth’s direction. It has already arrived, according to spacewather.com:

A CME struck Earth’s magnetic field during the late hours of September 6. So far the impact has done little to stoke strong geomagnetic activity. Another CME is on the way, however, and it is more potent, having been accelerated in our direction by yesterday’s powerful X9-class solar flare. NOAA forecasters say strong G3-class geomagnetic storms are possible on September 8 when the inbound CME arrives.

Reporting at skyandtelescope.com, Bob King wrote there may be a good shot at seeing the aurora borealis from the northern border states to as far south as Illinois and Oregon. But he said:

…the timing couldn’t be worse. It’s full moon and western skies are filled with smoke. A strong storm would likely still show up as bright arcs or balletic rays dancing across the northern sky. If AR2673 continues spouting flares, auroras could also appear later in the week, when the moon won’t be as much of a problem. That’s why I’d advise you to keep a lookout through the weekend.

Spaceweather.com agreed about watching for auroras through late week, adding:

Many readers are asking about the historic context of this event. How epic is it? Answer: This is a decade-class flare. A list of the most powerful solar flares recorded since 1976 ranks [the September 6] flare at #14, tied with a similar explosion in 1990. However, compared to the iconic Carrington Event of 1859, or even the more recent Halloween storms of 2003, this event is relatively mild. Modern power grids, telecommunications, and other sun sensitive technologies should weather the storm with little difficulty.

On the other hand, sky watchers could see some fantastic auroras before the week is over. And ham radio operators will surely be noticing strange propagation effects as the sun exerts its influence on our planet’s ionosphere.

Gowrishankar Lakshminarayanan captured this sunset on September 4, 2017 and called it: “… a surreal sunset from Fire Island Lighthouse in Fire Island, New York. You can see the 2 giant sunspots – AR2673 and AR2674 – as the sun is setting.”

Bottom line: It’s been a week of giant sunspots and solar flares! Watch for auroras into this weekend.



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Extreme UV flash from the powerful X9.3-class solar flare on September 6. Spaceweather.com called it “a decade-class flare.” Image via NASA SDO.

Sure, we’re headed toward solar minimum, but that didn’t keep the sun from acting up this week. Since last weekend, two gigantic sunspots – AR2673 and its pal AR2674 – have been seen from around the world by those using safe solar filters. They’ve been seen even with the (safely filtered) eye alone, making their way across the sun’s face. These Active Regions on the sun spawned multiple moderate (M-class) flares on September 4 and 5. Then yesterday – on September 6, 2017 – sunspot AR2673 erupted in a powerful X9.3-class solar flare, the strongest solar flare in more than a decade. Spaceweather.com reported the X-rays and UV radiation from the blast ionized the top of Earth’s atmosphere, causing a strong shortwave radio blackout over Europe, Africa and the Atlantic Ocean.

In the process of emitting the flares, AR2673 also blasted a coronal mass ejection (CME) into space in Earth’s direction. It has already arrived, according to spacewather.com:

A CME struck Earth’s magnetic field during the late hours of September 6. So far the impact has done little to stoke strong geomagnetic activity. Another CME is on the way, however, and it is more potent, having been accelerated in our direction by yesterday’s powerful X9-class solar flare. NOAA forecasters say strong G3-class geomagnetic storms are possible on September 8 when the inbound CME arrives.

Reporting at skyandtelescope.com, Bob King wrote there may be a good shot at seeing the aurora borealis from the northern border states to as far south as Illinois and Oregon. But he said:

…the timing couldn’t be worse. It’s full moon and western skies are filled with smoke. A strong storm would likely still show up as bright arcs or balletic rays dancing across the northern sky. If AR2673 continues spouting flares, auroras could also appear later in the week, when the moon won’t be as much of a problem. That’s why I’d advise you to keep a lookout through the weekend.

Spaceweather.com agreed about watching for auroras through late week, adding:

Many readers are asking about the historic context of this event. How epic is it? Answer: This is a decade-class flare. A list of the most powerful solar flares recorded since 1976 ranks [the September 6] flare at #14, tied with a similar explosion in 1990. However, compared to the iconic Carrington Event of 1859, or even the more recent Halloween storms of 2003, this event is relatively mild. Modern power grids, telecommunications, and other sun sensitive technologies should weather the storm with little difficulty.

On the other hand, sky watchers could see some fantastic auroras before the week is over. And ham radio operators will surely be noticing strange propagation effects as the sun exerts its influence on our planet’s ionosphere.

Gowrishankar Lakshminarayanan captured this sunset on September 4, 2017 and called it: “… a surreal sunset from Fire Island Lighthouse in Fire Island, New York. You can see the 2 giant sunspots – AR2673 and AR2674 – as the sun is setting.”

Bottom line: It’s been a week of giant sunspots and solar flares! Watch for auroras into this weekend.



from EarthSky http://ift.tt/2wKFwkL

Asteroid spacecraft to slingshot past Earth

Artist’s concept of OSIRIS-REx mission to asteroid Bennu, via NASA Goddard Spaceflight Center.

OSIRIS-REx is a space mission, the first of its kind for NASA, whose goal is to rendezvous with an asteroid and ultimately return a sample from it. The craft, which launched from Earth one year ago – and which is due to arrive at asteroid Bennu in 2018 – will soon use Earth’s gravity to give it a momentum boost toward its goal. The maneuver is called a gravity assist or a gravity slingshot. The spacecraft will pass about 11,000 miles (17,000 km) above Earth just before 16:52 p.m. UTC on September 22 (translate to your time zone). It’ll come just close enough to Earth to to be slung back to space – via Earth’s gravity – on a different trajectory and with a greater speed than before.

How to spot OSIRIS-REx on its September 22 flyover, and submit images

OSIRIS-REx stands for Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer. Big name, and it’s a big mission because, so far, humanity has collected samples of five worlds in our solar system, other than Earth. There are the moon rocks, of course. Unmanned spacecraft have also visited a comet, Wild 2 – and another asteroid, 25143 Itokawa – and returned samples to Earth. Plus scientists believe we have samples of the asteroid Vesta, and the planet Mars, in the form of meteorites that have fallen to Earth from space.

OSIRIS-REx’s mission is to rendezvous with asteroid Bennu, survey its surface, collect samples and deliver them safely back to Earth.

But first it has to get there. Bennu’s orbit around the sun is tilted six degrees in comparison to Earth’s. The gravity assist will change OSIRIS-REx’s trajectory to put the spacecraft on a course to match the asteroid’s path and speed. Dante Lauretta, OSIRIS-REx principal investigator at the University of Arizona, said in a statement:

The Earth gravity assist is a clever way to move the spacecraft onto Bennu’s orbital plane using Earth’s own gravity instead of expending fuel.

The mission is inviting the public to mark the OSIRIS-REX flyover by participating in a Wave to OSIRIS-REx social media campaign. Individuals and groups from anywhere in the world are encouraged to take photos of themselves waving to OSIRIS-REx, share them using the hashtag #HelloOSIRISREx and tag the mission account in their posts on Twitter (@OSIRISREx) or Instagram (@OSIRIS_REx). NASA said:

Participants may begin taking and sharing photos at any time—or wait until the OSIRIS-REx spacecraft makes its closest approach to Earth at 12:52p.m. EDT on Friday, September 22.

The NASA statement also explained:

The team has already made multiple adjustments to the spacecraft’s path since launch on September 8, 2016. The largest was a deep space maneuver on December 28, 2016, that changed the speed and path of the spacecraft to target Earth for the flyby. There have also been three trajectory correction maneuvers – one on October 7, 2016, one on January 18, 2017, and another on August 23, 2017 (30 days before the gravity assist) – that further refined the spacecraft’s trajectory in preparation for the flyby …

To properly target the Earth gravity assist, the navigation team calculates any required amount of change in the spacecraft’s course and speed. This information is then translated by the operations team into commands that are uploaded to the spacecraft and executed by firing the spacecraft’s rocket engines.

After traveling almost 600 million miles [nearly a billion km], OSIRIS-REx will approach Earth at a speed of about 19,000 mph [30,000 kph]. The spacecraft will fly over Australia before reaching its closest point to Earth over Antarctica, just south of Cape Horn, Chile.

Mike Moreau, the flight dynamics system lead at NASA’s Goddard Spaceflight Center, said:

For about an hour, NASA will be out of contact with the spacecraft as it passes over Antarctica. OSIRIS-REx uses the Deep Space Network to communicate with Earth, and the spacecraft will be too low relative to the southern horizon to be in view with either the Deep Space tracking station at Canberra, Australia, or Goldstone, California.

NASA will regain communication with OSIRIS-REx at 17:40 p.m. UTC, roughly 50 minutes after closest approach (translate to your time zone).

At 20:52 p.m. UTC, four hours after closest approach, OSIRIS-REx will begin science observations of Earth and the moon to calibrate its instruments.

Read more from NASA Goddard Spaceflight Center

Bottom line: NASA’s asteroid sample return mission, OSIRIS-REx, will undergo a gravity assist from Earth on September 22, 2017, passing about 11,000 miles (17,000 km) above our world. The momentum boost will help the craft reach asteroid Bennu in 2018, in a sample return mission.



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Artist’s concept of OSIRIS-REx mission to asteroid Bennu, via NASA Goddard Spaceflight Center.

OSIRIS-REx is a space mission, the first of its kind for NASA, whose goal is to rendezvous with an asteroid and ultimately return a sample from it. The craft, which launched from Earth one year ago – and which is due to arrive at asteroid Bennu in 2018 – will soon use Earth’s gravity to give it a momentum boost toward its goal. The maneuver is called a gravity assist or a gravity slingshot. The spacecraft will pass about 11,000 miles (17,000 km) above Earth just before 16:52 p.m. UTC on September 22 (translate to your time zone). It’ll come just close enough to Earth to to be slung back to space – via Earth’s gravity – on a different trajectory and with a greater speed than before.

How to spot OSIRIS-REx on its September 22 flyover, and submit images

OSIRIS-REx stands for Origins, Spectral Interpretation, Resource Identification, and Security – Regolith Explorer. Big name, and it’s a big mission because, so far, humanity has collected samples of five worlds in our solar system, other than Earth. There are the moon rocks, of course. Unmanned spacecraft have also visited a comet, Wild 2 – and another asteroid, 25143 Itokawa – and returned samples to Earth. Plus scientists believe we have samples of the asteroid Vesta, and the planet Mars, in the form of meteorites that have fallen to Earth from space.

OSIRIS-REx’s mission is to rendezvous with asteroid Bennu, survey its surface, collect samples and deliver them safely back to Earth.

But first it has to get there. Bennu’s orbit around the sun is tilted six degrees in comparison to Earth’s. The gravity assist will change OSIRIS-REx’s trajectory to put the spacecraft on a course to match the asteroid’s path and speed. Dante Lauretta, OSIRIS-REx principal investigator at the University of Arizona, said in a statement:

The Earth gravity assist is a clever way to move the spacecraft onto Bennu’s orbital plane using Earth’s own gravity instead of expending fuel.

The mission is inviting the public to mark the OSIRIS-REX flyover by participating in a Wave to OSIRIS-REx social media campaign. Individuals and groups from anywhere in the world are encouraged to take photos of themselves waving to OSIRIS-REx, share them using the hashtag #HelloOSIRISREx and tag the mission account in their posts on Twitter (@OSIRISREx) or Instagram (@OSIRIS_REx). NASA said:

Participants may begin taking and sharing photos at any time—or wait until the OSIRIS-REx spacecraft makes its closest approach to Earth at 12:52p.m. EDT on Friday, September 22.

The NASA statement also explained:

The team has already made multiple adjustments to the spacecraft’s path since launch on September 8, 2016. The largest was a deep space maneuver on December 28, 2016, that changed the speed and path of the spacecraft to target Earth for the flyby. There have also been three trajectory correction maneuvers – one on October 7, 2016, one on January 18, 2017, and another on August 23, 2017 (30 days before the gravity assist) – that further refined the spacecraft’s trajectory in preparation for the flyby …

To properly target the Earth gravity assist, the navigation team calculates any required amount of change in the spacecraft’s course and speed. This information is then translated by the operations team into commands that are uploaded to the spacecraft and executed by firing the spacecraft’s rocket engines.

After traveling almost 600 million miles [nearly a billion km], OSIRIS-REx will approach Earth at a speed of about 19,000 mph [30,000 kph]. The spacecraft will fly over Australia before reaching its closest point to Earth over Antarctica, just south of Cape Horn, Chile.

Mike Moreau, the flight dynamics system lead at NASA’s Goddard Spaceflight Center, said:

For about an hour, NASA will be out of contact with the spacecraft as it passes over Antarctica. OSIRIS-REx uses the Deep Space Network to communicate with Earth, and the spacecraft will be too low relative to the southern horizon to be in view with either the Deep Space tracking station at Canberra, Australia, or Goldstone, California.

NASA will regain communication with OSIRIS-REx at 17:40 p.m. UTC, roughly 50 minutes after closest approach (translate to your time zone).

At 20:52 p.m. UTC, four hours after closest approach, OSIRIS-REx will begin science observations of Earth and the moon to calibrate its instruments.

Read more from NASA Goddard Spaceflight Center

Bottom line: NASA’s asteroid sample return mission, OSIRIS-REx, will undergo a gravity assist from Earth on September 22, 2017, passing about 11,000 miles (17,000 km) above our world. The momentum boost will help the craft reach asteroid Bennu in 2018, in a sample return mission.



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How to see the Great Square of Pegasus

Image via astrobob.

How to find it

The Great Square of Pegasus gallops into the fall sky just after dark around the September equinox, which falls in 2017 on September 22. Look to the east to northeast just above the horizon. If you are in dark skies, the river of stars known as the Milky Way streams overhead through the Summer Triangle.

Great Square of Pegasus

Four stars of nearly equal brightness make up the Great Square of Pegasus: Scheat, Alpheratz, Markab and Algenib. A landmark of the Northern Hemisphere’s autumn sky, it looks like a celestial baseball diamond or a great big square. To find it, first of all use the Big Dipper to star-hop to Polaris the North Star. By drawing an imaginary line from any Big Dipper handle star through Polaris, and going twice the distance, you’ll always land on the W or M-shaped constellation Cassiopeia the Queen. A line from Polaris through the star Caph of Cassiopeia faithfully escorts you to the Great Square of Pegasus.

Sky chart of Pegasus and Great Square

The Great Square of Pegasus makes up the eastern (left) half of the constellation Pegasus. Image credit: Wikimedia Commons

The Great Square is used much like the Big Dipper to help you find other sky treasures, the most notable being the Andromeda Galaxy. Also, like the Big Dipper, the Great Square of Pegasus is an asterism or part of a constellation. The four second-magnitude stars that make up the square are Scheat, Alpheratz, Markab and Algenib.

A great big square of nothing

Often at events where many are stargazing for the first time, one may hear, “this great big square has nothing in it.” The square isn’t exactly empty. The stars in the square are faint enough that the unaided eye can’t easily detect them. If you have binoculars or small telescopes many stars pop up within the square.

One of the most famous faint stars near the Great Square is 51 Pegasi. In 1995 astronomers announced they discovered a planet around this star. After a few months of skepticism from the astronomical community, it was confirmed the first planet outside of our solar system was discovered. Now we know that two planets orbit the star. Some books say that 51 Pegasi is naked-eye but it is a bit of a challenge. Using binoculars, look roughly halfway between Scheat and Markab. Here is a chart, courtesy of Professor Jim Kaler. Note that you won’t be able to see the planets. Pegasus 51 is approximately 50 light-years away from Earth.

Mythology

As one may remember, Pegasus was a winged horse in Greek mythology. The constellation Pegasus is one of seven constellations in the sky that tells why it is not good to say that a mortal is more beautiful than the gods. This story is plastered all over the autumn night sky.

Queen Cassiopeia bragged that she (or her daughter Andromeda) was more beautiful than immortal Nereids, or sea nymphs. This angered the gods, who asked the sea-god Poseidon to take revenge. The punishment was that King Cepheus and the Queen had to sacrifice their only daughter Andromeda to Cetus the sea monster. Andromeda while chained down to a rock at sea, and about to be gobbled up by the sea monster, saw Perseus riding Pegasus the flying horse. Perseus swooped down and showed the head of the Medusa to the Cetus, the sea monster, then Cetus immediately turned to stone. Then he whacked the chains holding Andromeda and freed her.

They flew off into the sunset to live happily ever after. The mortal horse on the last day of his life was given the honor of becoming a constellation for his loyal service. The dolphin that provided comfort to Andromeda was also granted immortality in the heavens by Zeus with the Delphinus constellation.

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Bottom line: How to see the Great Square of Pegasus star pattern.



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Image via astrobob.

How to find it

The Great Square of Pegasus gallops into the fall sky just after dark around the September equinox, which falls in 2017 on September 22. Look to the east to northeast just above the horizon. If you are in dark skies, the river of stars known as the Milky Way streams overhead through the Summer Triangle.

Great Square of Pegasus

Four stars of nearly equal brightness make up the Great Square of Pegasus: Scheat, Alpheratz, Markab and Algenib. A landmark of the Northern Hemisphere’s autumn sky, it looks like a celestial baseball diamond or a great big square. To find it, first of all use the Big Dipper to star-hop to Polaris the North Star. By drawing an imaginary line from any Big Dipper handle star through Polaris, and going twice the distance, you’ll always land on the W or M-shaped constellation Cassiopeia the Queen. A line from Polaris through the star Caph of Cassiopeia faithfully escorts you to the Great Square of Pegasus.

Sky chart of Pegasus and Great Square

The Great Square of Pegasus makes up the eastern (left) half of the constellation Pegasus. Image credit: Wikimedia Commons

The Great Square is used much like the Big Dipper to help you find other sky treasures, the most notable being the Andromeda Galaxy. Also, like the Big Dipper, the Great Square of Pegasus is an asterism or part of a constellation. The four second-magnitude stars that make up the square are Scheat, Alpheratz, Markab and Algenib.

A great big square of nothing

Often at events where many are stargazing for the first time, one may hear, “this great big square has nothing in it.” The square isn’t exactly empty. The stars in the square are faint enough that the unaided eye can’t easily detect them. If you have binoculars or small telescopes many stars pop up within the square.

One of the most famous faint stars near the Great Square is 51 Pegasi. In 1995 astronomers announced they discovered a planet around this star. After a few months of skepticism from the astronomical community, it was confirmed the first planet outside of our solar system was discovered. Now we know that two planets orbit the star. Some books say that 51 Pegasi is naked-eye but it is a bit of a challenge. Using binoculars, look roughly halfway between Scheat and Markab. Here is a chart, courtesy of Professor Jim Kaler. Note that you won’t be able to see the planets. Pegasus 51 is approximately 50 light-years away from Earth.

Mythology

As one may remember, Pegasus was a winged horse in Greek mythology. The constellation Pegasus is one of seven constellations in the sky that tells why it is not good to say that a mortal is more beautiful than the gods. This story is plastered all over the autumn night sky.

Queen Cassiopeia bragged that she (or her daughter Andromeda) was more beautiful than immortal Nereids, or sea nymphs. This angered the gods, who asked the sea-god Poseidon to take revenge. The punishment was that King Cepheus and the Queen had to sacrifice their only daughter Andromeda to Cetus the sea monster. Andromeda while chained down to a rock at sea, and about to be gobbled up by the sea monster, saw Perseus riding Pegasus the flying horse. Perseus swooped down and showed the head of the Medusa to the Cetus, the sea monster, then Cetus immediately turned to stone. Then he whacked the chains holding Andromeda and freed her.

They flew off into the sunset to live happily ever after. The mortal horse on the last day of his life was given the honor of becoming a constellation for his loyal service. The dolphin that provided comfort to Andromeda was also granted immortality in the heavens by Zeus with the Delphinus constellation.

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Bottom line: How to see the Great Square of Pegasus star pattern.



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