Last quarter moon is December 29

The moon was almost exactly at last quarter when Deirdre Horan in Dublin, Ireland, captured this photo. The terminator line, or line between light and dark on the moon, appears straight.

A last quarter moon appears half-lit by sunshine and half-immersed in its own shadow. It rises in the middle of the night, appears at its highest in the sky around dawn, and sets around midday. The moon reaches its exact half-illuminated phase, as viewed from Earth, on December 29, 2018, at 09:34 UTC; translate UTC to your time.

On a last quarter moon, the lunar terminator – the shadow line dividing day and night – shows you where it’s sunset on the moon.

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

The night before last quarter moon – on November 28, 2018 – the moon is near the bright star Regulus, Heart of the Lion in Leo. Day by day, before dawn, watch for the waning moon to sink toward Venus and to meet up with this dazzling world in early December 2018.

A last quarter moon provides a great opportunity to think of yourself on a three-dimensional world in space. For example, it’s fun to see this moon just after moonrise, shortly after midnight. Then the lighted portion points downward, to the sun below your feet. Think of the last quarter moon as a mirror to the world you’re standing on. Think of yourself standing in the middle of Earth’s nightside, on the midnight portion of Earth.

Also, a last quarter moon can be used as a guidepost to Earth’s direction of motion in orbit around the sun.

In other words, when you look toward a last quarter moon high in the predawn sky, for example, you’re gazing out approximately along the path of Earth’s orbit, in a forward direction. The moon is moving in orbit around the sun with the Earth and never holds still. But, if we could somehow anchor the moon in space … tie it down, keep it still … Earth’s orbital speed of 18 miles per second would carry us across the space between us and the moon in only a few hours.

Want to read more about the last quarter moon as a guidepost for Earth’s motion? Astronomer Guy Ottewell talked about it recently, too.

A great thing about using the moon as a guidepost to Earth’s motion is that you can do it anywhere … as, for example, in the photo below, from large cities.

Ben Orlove wrote from New York City: “I was sitting in the roof garden of my building, and there was the moon, right in front of me. You were right, this is a perfect time to visualize … the Earth’s motion.”

As the moon orbits Earth, it changes phase in an orderly way. Follow the links below to understand the phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

Read more: 4 keys to understanding moon phases

Bottom line: The next last quarter moon falls on December 29, 2018, at 09:34 UTC; translate UTC to your time.



from EarthSky http://bit.ly/2TgCmPT

The moon was almost exactly at last quarter when Deirdre Horan in Dublin, Ireland, captured this photo. The terminator line, or line between light and dark on the moon, appears straight.

A last quarter moon appears half-lit by sunshine and half-immersed in its own shadow. It rises in the middle of the night, appears at its highest in the sky around dawn, and sets around midday. The moon reaches its exact half-illuminated phase, as viewed from Earth, on December 29, 2018, at 09:34 UTC; translate UTC to your time.

On a last quarter moon, the lunar terminator – the shadow line dividing day and night – shows you where it’s sunset on the moon.

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

The night before last quarter moon – on November 28, 2018 – the moon is near the bright star Regulus, Heart of the Lion in Leo. Day by day, before dawn, watch for the waning moon to sink toward Venus and to meet up with this dazzling world in early December 2018.

A last quarter moon provides a great opportunity to think of yourself on a three-dimensional world in space. For example, it’s fun to see this moon just after moonrise, shortly after midnight. Then the lighted portion points downward, to the sun below your feet. Think of the last quarter moon as a mirror to the world you’re standing on. Think of yourself standing in the middle of Earth’s nightside, on the midnight portion of Earth.

Also, a last quarter moon can be used as a guidepost to Earth’s direction of motion in orbit around the sun.

In other words, when you look toward a last quarter moon high in the predawn sky, for example, you’re gazing out approximately along the path of Earth’s orbit, in a forward direction. The moon is moving in orbit around the sun with the Earth and never holds still. But, if we could somehow anchor the moon in space … tie it down, keep it still … Earth’s orbital speed of 18 miles per second would carry us across the space between us and the moon in only a few hours.

Want to read more about the last quarter moon as a guidepost for Earth’s motion? Astronomer Guy Ottewell talked about it recently, too.

A great thing about using the moon as a guidepost to Earth’s motion is that you can do it anywhere … as, for example, in the photo below, from large cities.

Ben Orlove wrote from New York City: “I was sitting in the roof garden of my building, and there was the moon, right in front of me. You were right, this is a perfect time to visualize … the Earth’s motion.”

As the moon orbits Earth, it changes phase in an orderly way. Follow the links below to understand the phases of the moon.

New moon
Waxing crescent moon
First quarter moon
Waxing gibbous moon
Full moon
Waning gibbous moon
Last quarter moon
Waning crescent moon

Read more: 4 keys to understanding moon phases

Bottom line: The next last quarter moon falls on December 29, 2018, at 09:34 UTC; translate UTC to your time.



from EarthSky http://bit.ly/2TgCmPT

Spacecraft spies ice-filled Mars crater

A stunning perspective view of the ice-filled Korolev Crater, as seen by Mars Express. Image via ESA/DLR/FU Berlin/BY-SA 3.0 IGO.

Mars is famous for its polar ice caps – composed of both water ice and carbon dioxide ice – which stand out starkly against the surrounding rust-colored terrain. But plentiful ice can be found outside of Mars’ main ice caps as well, including underground. One image in particular shows a beautiful example of such a Martian icy landscape – an “ice pond” in a crater near the north pole – very fitting for this time of year in the northern hemispheres of both Earth and Mars. That’s right … it’s winter in Mars’ northern hemisphere now, too. The Martian northern winter solstice came on October 16, 2018 (Mars seasonal calendar here).

The European Space Agency (ESA) acquired the image at top, and several other images on this page, via its Mars Express orbiter. The one above shows what at first looks like a scenic view of an untouched patch of Martian snow, but the brilliantly white feature is actually water ice, filling Mars’ Korolev Crater. The roundish mound of ice is captured in exquisite detail; notice the smaller patches of ice filling in crevices on the rugged edge of the crater rim. ESA posted the image on December 20, 2018.

Korolev Crater is about 51 miles (82 km) across and is located in the northern lowlands of Mars, just south of Olympia Undae – an expanse of dune-filled terrain that partially surrounds the north pole. The image shows a stunning oblique view of the crater, composed of five different “strips” combined to form a larger single image. Each strip was obtained during a different orbit by Mars Express. There are also context and topographic views of the crater.

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Image showing Korolev Crater and surrounding terrain, including the different image strips combined to create the larger perspective image. Image via NASA MGS MOLA Science Team.

The ice that fills the crater largely persists year-round – the central mound of ice maintains a thickness of 1.1 miles (1.8 km). The crater acts as a cold trap, where the air cools down and sinks as it moves over the ice deposit, creating a layer of cold air that sits directly above the ice itself. That cold layer keeps the ice stable and prevents it from evaporating or sublimating. The crater itself is quite deep, with the crater floor lying some 1.2 miles (2 km) beneath the crater rim.

Korolev Crater was also recently imaged – partially – by ESA’s Trace Gas Orbiter (TGO), part of the ExoMars mission. TGO arrived at Mars last spring, and is designed to search the Martian atmosphere for trace gases – tiny amounts of certain gases such as methane.

Ice is common on Mars – both on the surface and in the subsurface – including both water ice and carbon dioxide ice. NASA’s Phoenix lander dug into the frozen surface near the north pole back in 2008 and sampled some of the water ice directly, just a few inches below the surface. Phoenix also observed snow falling high up in the atmosphere, although it didn’t reach the ground. So there is snow on Mars as well, but it never accumulates enough to go skiing or sledding, unfortunately. On the other hand, ice-filled craters like Korolev might make somewhat-ideal skating rinks for some future Martian settlers!

An overhead view of Korolev Crater. Image via ESA/DLR/FU Berlin/CC BY-SA 3.0 IGO.

Color-coded image showing the topography of Korolev Crater. Lower parts of the surface are shown in blues and purples, while higher-altitude regions are shown in whites, browns and reds, as indicated on the scale to the top right. Image via ESA/DLR/FU Berlin/CC BY-SA 3.0 IGO.

Part of the rim of Korolev Crater, as seen by the Colour and Stereo Surface Imaging System (CaSSIS) on Mars Express. Image via ESA/Roscosmos/CaSSIS.

Korolev Crater was named after Sergei Korolev, a chief rocket engineer and spacecraft designer who was dubbed the father of Soviet space technology.

Mars Express was launched way back in 2003 and entered Mars orbit on December 25 of the same year – 15 years ago this week!

More information about Mars Express is available on the mission website.

Bottom line: The “frozen pond” in Korolev Crater is a beautiful example of how the cold, icy terrain on Mars can be reminiscent of similar places on Earth –  a Martian winter wonderland.

Via ESA



from EarthSky http://bit.ly/2RpaNqs

A stunning perspective view of the ice-filled Korolev Crater, as seen by Mars Express. Image via ESA/DLR/FU Berlin/BY-SA 3.0 IGO.

Mars is famous for its polar ice caps – composed of both water ice and carbon dioxide ice – which stand out starkly against the surrounding rust-colored terrain. But plentiful ice can be found outside of Mars’ main ice caps as well, including underground. One image in particular shows a beautiful example of such a Martian icy landscape – an “ice pond” in a crater near the north pole – very fitting for this time of year in the northern hemispheres of both Earth and Mars. That’s right … it’s winter in Mars’ northern hemisphere now, too. The Martian northern winter solstice came on October 16, 2018 (Mars seasonal calendar here).

The European Space Agency (ESA) acquired the image at top, and several other images on this page, via its Mars Express orbiter. The one above shows what at first looks like a scenic view of an untouched patch of Martian snow, but the brilliantly white feature is actually water ice, filling Mars’ Korolev Crater. The roundish mound of ice is captured in exquisite detail; notice the smaller patches of ice filling in crevices on the rugged edge of the crater rim. ESA posted the image on December 20, 2018.

Korolev Crater is about 51 miles (82 km) across and is located in the northern lowlands of Mars, just south of Olympia Undae – an expanse of dune-filled terrain that partially surrounds the north pole. The image shows a stunning oblique view of the crater, composed of five different “strips” combined to form a larger single image. Each strip was obtained during a different orbit by Mars Express. There are also context and topographic views of the crater.

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

Image showing Korolev Crater and surrounding terrain, including the different image strips combined to create the larger perspective image. Image via NASA MGS MOLA Science Team.

The ice that fills the crater largely persists year-round – the central mound of ice maintains a thickness of 1.1 miles (1.8 km). The crater acts as a cold trap, where the air cools down and sinks as it moves over the ice deposit, creating a layer of cold air that sits directly above the ice itself. That cold layer keeps the ice stable and prevents it from evaporating or sublimating. The crater itself is quite deep, with the crater floor lying some 1.2 miles (2 km) beneath the crater rim.

Korolev Crater was also recently imaged – partially – by ESA’s Trace Gas Orbiter (TGO), part of the ExoMars mission. TGO arrived at Mars last spring, and is designed to search the Martian atmosphere for trace gases – tiny amounts of certain gases such as methane.

Ice is common on Mars – both on the surface and in the subsurface – including both water ice and carbon dioxide ice. NASA’s Phoenix lander dug into the frozen surface near the north pole back in 2008 and sampled some of the water ice directly, just a few inches below the surface. Phoenix also observed snow falling high up in the atmosphere, although it didn’t reach the ground. So there is snow on Mars as well, but it never accumulates enough to go skiing or sledding, unfortunately. On the other hand, ice-filled craters like Korolev might make somewhat-ideal skating rinks for some future Martian settlers!

An overhead view of Korolev Crater. Image via ESA/DLR/FU Berlin/CC BY-SA 3.0 IGO.

Color-coded image showing the topography of Korolev Crater. Lower parts of the surface are shown in blues and purples, while higher-altitude regions are shown in whites, browns and reds, as indicated on the scale to the top right. Image via ESA/DLR/FU Berlin/CC BY-SA 3.0 IGO.

Part of the rim of Korolev Crater, as seen by the Colour and Stereo Surface Imaging System (CaSSIS) on Mars Express. Image via ESA/Roscosmos/CaSSIS.

Korolev Crater was named after Sergei Korolev, a chief rocket engineer and spacecraft designer who was dubbed the father of Soviet space technology.

Mars Express was launched way back in 2003 and entered Mars orbit on December 25 of the same year – 15 years ago this week!

More information about Mars Express is available on the mission website.

Bottom line: The “frozen pond” in Korolev Crater is a beautiful example of how the cold, icy terrain on Mars can be reminiscent of similar places on Earth –  a Martian winter wonderland.

Via ESA



from EarthSky http://bit.ly/2RpaNqs

What does Ceres’ carbon mean?

False-color image of dwarf planet Ceres – largest body in the asteroid belt – from the Dawn spacecraft. The image shows Ceres’ famous bright spots, and the false color highlights differences in surface materials. Image via NASA PhotoJournal.

Carbon is one of the most common elements in the universe and is the basis of organic biology on Earth. It can be found throughout the solar system, even in meteorites that bounce to Earth’s surface from other parts of space. Now scientists have found that another body in the solar system – the dwarf planet Ceres – is much richer in carbon that previously thought. Those results were published in a peer-reviewed article in Nature Astronomy on December 10, 2018.

Astronomer Simone Marchi at Southwest Research Institute (SwRI) was the lead author of the new paper. He said:

Ceres is like a chemical factory. Among inner solar system bodies, Ceres has a unique mineralogy, which appears to contain up to 20 percent carbon by mass in its near surface. Our analysis shows that carbon-rich compounds are intimately mixed with products of rock-water interactions, such as clays.

The interior structure of Ceres as scientists now understand it. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA.

Why is the presence of carbon so intriguing? Carbon isn’t by itself necessarily the product of or connected to life, although it does serve as the basis for organic chemistry and biology on Earth. When combined with oxygen and hydrogen, carbon can form many groups of important biological compounds including sugars, alcohols and fats. Its presence on Ceres is evidence that the basic ingredients for life – including carbon – can be found in many different places, not only in our solar system but throughout the universe.

More specifically, the new findings show that Ceres was, and still is, rich in amorphous carbon – a carbon-rich organic material – which is significant in terms of how carbon is distributed throughout the solar system. (Organic materials are any molecules that contain carbon – they can be formed on their own without life but are also building blocks of life). The new data suggests that Ceres contains several times more amorphous carbon on its surface and in its subsurface than even the most carbon-rich meteorites.

While Ceres contains more carbon than meteorites, the study also shows that 50 to 60 percent of Ceres’ upper crust may have a composition similar to primitive carbonaceous chondrite meteorites – some of the most complex of all meteorites.

Close-up view inside Urvara crater on Ceres. The 6,500-foot (1981-meter) central ridge is made from materials uplifted from deep below the surface, which experienced rock-water chemical interactions. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA.

As Marchi explained:

Our results imply that either Ceres accreted ultra-carbon-rich materials or that carbon was concentrated in its crust. Both potential scenarios are important, because Ceres’ mineralogical composition indicates a global-scale event of rock-water alteration, which could provide conditions favorable to organic chemistry.

In other words, the carbon on Ceres may originate from when Ceres first formed or from incoming impacts of other asteroids. Scientists don’t know yet which scenario is correct. But regardless, the evidence for chemical reactions with water is intriguing, since that can eventually lead to the formation of the building blocks of life, even if not life itself.

Ceres is classified as a dwarf planet but is also the largest asteroid in the main asteroid belt between Mars and Jupiter. NASA’s Dawn spacecraft recently finished its mission at Ceres on November 1, 2018, studying its geology and sending back incredible high-resolution images of its surface from orbit. One big surprise was the “bright spots” – light-colored deposits, now determined to be sodium carbonate salts – on the darker rocky surface. Scientists think they were formed when when water came up to the surface from deeper below and then evaporated in Ceres’ extremely tenuous and sporadic water vapor “atmosphere.”

The best-known bright spots are those in Occator Crater, which stand out starkly against the darker rocky surface.

High-resolution view of Cerealia Facula – a sodium carbonate (salt) deposit – in Occator Crater. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/Roman Tkachenko.

Whether Ceres ever had conditions suitable for life to evolve is still unknown, although there is also evidence that it has, or at least once had, water below the surface – maybe even a subsurface ocean. This water produced chemical reactions when it came in contact with minerals in rocks. There is also evidence for past cryovolcanic activity – cryovolcanoes, which erupt water, ammonia or methane rather than molten rock. It’s even possible that the subsurface environment was once warm and wet enough for basic biological chemistry to actually begin, although no direct signs of that have been discovered yet.

Bottom line: As the largest object in the asteroid belt, Ceres is a fascinating world, and has been more geologically active than previously thought. The fact that Ceres is rich in organic carbon is a big part of its geological history and now scientists are beginning to understand what that means not only for the widespread presence of carbon in the solar system but also how organic chemistry can – at least sometimes – lead to the development of life itself.

Source: An aqueously altered carbon-rich Ceres

Via SwRI

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from EarthSky http://bit.ly/2ERwQju

False-color image of dwarf planet Ceres – largest body in the asteroid belt – from the Dawn spacecraft. The image shows Ceres’ famous bright spots, and the false color highlights differences in surface materials. Image via NASA PhotoJournal.

Carbon is one of the most common elements in the universe and is the basis of organic biology on Earth. It can be found throughout the solar system, even in meteorites that bounce to Earth’s surface from other parts of space. Now scientists have found that another body in the solar system – the dwarf planet Ceres – is much richer in carbon that previously thought. Those results were published in a peer-reviewed article in Nature Astronomy on December 10, 2018.

Astronomer Simone Marchi at Southwest Research Institute (SwRI) was the lead author of the new paper. He said:

Ceres is like a chemical factory. Among inner solar system bodies, Ceres has a unique mineralogy, which appears to contain up to 20 percent carbon by mass in its near surface. Our analysis shows that carbon-rich compounds are intimately mixed with products of rock-water interactions, such as clays.

The interior structure of Ceres as scientists now understand it. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA.

Why is the presence of carbon so intriguing? Carbon isn’t by itself necessarily the product of or connected to life, although it does serve as the basis for organic chemistry and biology on Earth. When combined with oxygen and hydrogen, carbon can form many groups of important biological compounds including sugars, alcohols and fats. Its presence on Ceres is evidence that the basic ingredients for life – including carbon – can be found in many different places, not only in our solar system but throughout the universe.

More specifically, the new findings show that Ceres was, and still is, rich in amorphous carbon – a carbon-rich organic material – which is significant in terms of how carbon is distributed throughout the solar system. (Organic materials are any molecules that contain carbon – they can be formed on their own without life but are also building blocks of life). The new data suggests that Ceres contains several times more amorphous carbon on its surface and in its subsurface than even the most carbon-rich meteorites.

While Ceres contains more carbon than meteorites, the study also shows that 50 to 60 percent of Ceres’ upper crust may have a composition similar to primitive carbonaceous chondrite meteorites – some of the most complex of all meteorites.

Close-up view inside Urvara crater on Ceres. The 6,500-foot (1981-meter) central ridge is made from materials uplifted from deep below the surface, which experienced rock-water chemical interactions. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA.

As Marchi explained:

Our results imply that either Ceres accreted ultra-carbon-rich materials or that carbon was concentrated in its crust. Both potential scenarios are important, because Ceres’ mineralogical composition indicates a global-scale event of rock-water alteration, which could provide conditions favorable to organic chemistry.

In other words, the carbon on Ceres may originate from when Ceres first formed or from incoming impacts of other asteroids. Scientists don’t know yet which scenario is correct. But regardless, the evidence for chemical reactions with water is intriguing, since that can eventually lead to the formation of the building blocks of life, even if not life itself.

Ceres is classified as a dwarf planet but is also the largest asteroid in the main asteroid belt between Mars and Jupiter. NASA’s Dawn spacecraft recently finished its mission at Ceres on November 1, 2018, studying its geology and sending back incredible high-resolution images of its surface from orbit. One big surprise was the “bright spots” – light-colored deposits, now determined to be sodium carbonate salts – on the darker rocky surface. Scientists think they were formed when when water came up to the surface from deeper below and then evaporated in Ceres’ extremely tenuous and sporadic water vapor “atmosphere.”

The best-known bright spots are those in Occator Crater, which stand out starkly against the darker rocky surface.

High-resolution view of Cerealia Facula – a sodium carbonate (salt) deposit – in Occator Crater. Image via NASA/JPL-Caltech/UCLA/MPS/DLR/IDA/Roman Tkachenko.

Whether Ceres ever had conditions suitable for life to evolve is still unknown, although there is also evidence that it has, or at least once had, water below the surface – maybe even a subsurface ocean. This water produced chemical reactions when it came in contact with minerals in rocks. There is also evidence for past cryovolcanic activity – cryovolcanoes, which erupt water, ammonia or methane rather than molten rock. It’s even possible that the subsurface environment was once warm and wet enough for basic biological chemistry to actually begin, although no direct signs of that have been discovered yet.

Bottom line: As the largest object in the asteroid belt, Ceres is a fascinating world, and has been more geologically active than previously thought. The fact that Ceres is rich in organic carbon is a big part of its geological history and now scientists are beginning to understand what that means not only for the widespread presence of carbon in the solar system but also how organic chemistry can – at least sometimes – lead to the development of life itself.

Source: An aqueously altered carbon-rich Ceres

Via SwRI

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See brightest star Sirius at midnight on New Year’s Eve

Brightest star Sirius at culmination, or highest in the sky, via Project Nightflight. Note that “highest in the sky” doesn’t necessarily means “overhead.” Sirius’ height in your sky will depend on your latitude.

Want to surprise and impress your friends on New Year’s Eve? Show them Sirius, the brightest star in the sky, sometimes called the Dog Star because it’s part of the constellation Canis Major the Greater Dog. Sirius might also be called the New Year’s star. It’ll celebrate the birth of 2019 and every new year by reaching its highest point in the sky around the stroke of midnight. That’s the case this year, and every year.

How can you find Sirius? It’s easy because this star is the brightest one we see from Earth. Its name means sparkling or scorching.

If you look for the sky’s brightest star, and are still not sure, here’s a sure-fire way to identify it. Just look for the prominent Belt stars of the constellation Orion. Orion’s Belt always points to Sirius.

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You can always recognize Sirius, because the 3 noticeable stars in Orion’s Belt point to it.

This photo comes from EarthSky Facebook friend Susan Jensen in Odessa, Washington. See how it matches the chart above, with the 3 stars of Orion’s Belt pointing to Sirius?

So Sirius is highest in the sky at midnight every New Year’s. Astronomers call this a midnight culmination of Sirius. As the New Year rings in, Sirius is at its highest.

By midnight, by the way, we mean the middle of the night – midway between sunset and sunrise. Like the sun, the stars rise in the east and travel westward across the sky. When the sun or any star is in the eastern half of the sky, it’s climbing upward. When the sun or any star is in the western sky, it’s descending downward. Midway between rising and setting, the sun or any star reaches its highest point in the sky.

Because the stars rise and set two hours earlier with each passing month, Sirius will be highest up for the night around 10 p.m. local time on February 1.

Sirius from space. It’s the brightest star in this image, the bluish one, to the right in the photo. The 3 Belt stars of Orion – buried in the haze along Earth’s horizon – are still pointing to it.

Bottom line: Look for the star Sirius at midnight culmination – highest in the sky around midnight, or midway between sunset and sunrise – every New Year’s Eve.



from EarthSky http://bit.ly/2ER4FR8

Brightest star Sirius at culmination, or highest in the sky, via Project Nightflight. Note that “highest in the sky” doesn’t necessarily means “overhead.” Sirius’ height in your sky will depend on your latitude.

Want to surprise and impress your friends on New Year’s Eve? Show them Sirius, the brightest star in the sky, sometimes called the Dog Star because it’s part of the constellation Canis Major the Greater Dog. Sirius might also be called the New Year’s star. It’ll celebrate the birth of 2019 and every new year by reaching its highest point in the sky around the stroke of midnight. That’s the case this year, and every year.

How can you find Sirius? It’s easy because this star is the brightest one we see from Earth. Its name means sparkling or scorching.

If you look for the sky’s brightest star, and are still not sure, here’s a sure-fire way to identify it. Just look for the prominent Belt stars of the constellation Orion. Orion’s Belt always points to Sirius.

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

You can always recognize Sirius, because the 3 noticeable stars in Orion’s Belt point to it.

This photo comes from EarthSky Facebook friend Susan Jensen in Odessa, Washington. See how it matches the chart above, with the 3 stars of Orion’s Belt pointing to Sirius?

So Sirius is highest in the sky at midnight every New Year’s. Astronomers call this a midnight culmination of Sirius. As the New Year rings in, Sirius is at its highest.

By midnight, by the way, we mean the middle of the night – midway between sunset and sunrise. Like the sun, the stars rise in the east and travel westward across the sky. When the sun or any star is in the eastern half of the sky, it’s climbing upward. When the sun or any star is in the western sky, it’s descending downward. Midway between rising and setting, the sun or any star reaches its highest point in the sky.

Because the stars rise and set two hours earlier with each passing month, Sirius will be highest up for the night around 10 p.m. local time on February 1.

Sirius from space. It’s the brightest star in this image, the bluish one, to the right in the photo. The 3 Belt stars of Orion – buried in the haze along Earth’s horizon – are still pointing to it.

Bottom line: Look for the star Sirius at midnight culmination – highest in the sky around midnight, or midway between sunset and sunrise – every New Year’s Eve.



from EarthSky http://bit.ly/2ER4FR8

Most popular photos 2018

2018’s New Year’s supermoon: It was a great way to start 2018! The year started with a full moon that happened also to be the year’s closest and brightest supermoon. See photos.

Neeti Kumthekar in Belmar, New Jersey, caught the January 2018 supermoon rising with a mirage effect. The rising or setting moon or sun can exhibit a mirage when there are air layers of different temperatures near your horizon – for example, over an ocean. Read more about mirages from Atmospheric Optics.

Late April moon and Jupiter: The moon swept past the very bright planet Jupiter in late April, shortly before the giant planet was at its closest and brightest for the year. See photos.

Full moon and Jupiter – April 29, 2018 – shining through the hazy night over Oklahoma, captured by Mike O’Neal.

Full moon eclipse and Mars in late July: Mars was brighter in late July than it had been since 2003. Then – on July 27 – that very bright Mars appeared near the moon as it was undergoing a total eclipse. See photos.

Prabhakaran A wrote from Trichy, India: “The full moon on the night of July 27-28, 2018, presented the longest and darkest total lunar eclipse of the 21st century. Totality spanned 1 hour 42 minutes and 57 seconds. The most distant and smallest full moon of the year passed through the center of the Earth’s dark umbral shadow which reached its maximum length and width for the year. This beautiful eclipse happened on the same night of Mars opposition.”

Favorite Perseid meteor shower photos: 2018 was an exceptional year for August’s tried and true Perseid meteor shower. See photos.

Nicholas Holshouser wrote: “The Jerry Lee Lewis Memorial ‘Great Ball of Fire’ Perseid meteor. Looking west towards the Great Smoky Mountains from an overlook on the Blue Ridge Parkway. Taken at 4:38 a.m. on August 13, 2018. The bright train was visible for over a minute and it formed a high vapor cloud and was visible above me for more than 20 minutes as it went overhead.”

SpaceX’s cool night launch and landing on October 7: Night launches are always fun, and this October 7 launch by SpaceX – from Vandenberg Air Force Base, north of Los Angeles, California – generated more than its fair share of awesome images. See photos.

Allan Der sent in this photo from Downey, California, on October 7, 2018: “SpaceX Falcon 9 first stage rocket. I was not expecting to shoot the event, but happen to have my camera handy.”

See it! Images of comet 46P/Wirtanen: Look here for photos and video of 2018’s Christmas comet and brightest comet 46P/Wirtanen. See photos.

Comet 46P/Wirtanen on December 15, 2018 – hours before it came closest to Earth – via Juan Gonzalez-Alicea in Cabo Rojo, Puerto Rico.

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Bottom line: Most popular EarthSky photos from 2018.



from EarthSky http://bit.ly/2Ais4aV

2018’s New Year’s supermoon: It was a great way to start 2018! The year started with a full moon that happened also to be the year’s closest and brightest supermoon. See photos.

Neeti Kumthekar in Belmar, New Jersey, caught the January 2018 supermoon rising with a mirage effect. The rising or setting moon or sun can exhibit a mirage when there are air layers of different temperatures near your horizon – for example, over an ocean. Read more about mirages from Atmospheric Optics.

Late April moon and Jupiter: The moon swept past the very bright planet Jupiter in late April, shortly before the giant planet was at its closest and brightest for the year. See photos.

Full moon and Jupiter – April 29, 2018 – shining through the hazy night over Oklahoma, captured by Mike O’Neal.

Full moon eclipse and Mars in late July: Mars was brighter in late July than it had been since 2003. Then – on July 27 – that very bright Mars appeared near the moon as it was undergoing a total eclipse. See photos.

Prabhakaran A wrote from Trichy, India: “The full moon on the night of July 27-28, 2018, presented the longest and darkest total lunar eclipse of the 21st century. Totality spanned 1 hour 42 minutes and 57 seconds. The most distant and smallest full moon of the year passed through the center of the Earth’s dark umbral shadow which reached its maximum length and width for the year. This beautiful eclipse happened on the same night of Mars opposition.”

Favorite Perseid meteor shower photos: 2018 was an exceptional year for August’s tried and true Perseid meteor shower. See photos.

Nicholas Holshouser wrote: “The Jerry Lee Lewis Memorial ‘Great Ball of Fire’ Perseid meteor. Looking west towards the Great Smoky Mountains from an overlook on the Blue Ridge Parkway. Taken at 4:38 a.m. on August 13, 2018. The bright train was visible for over a minute and it formed a high vapor cloud and was visible above me for more than 20 minutes as it went overhead.”

SpaceX’s cool night launch and landing on October 7: Night launches are always fun, and this October 7 launch by SpaceX – from Vandenberg Air Force Base, north of Los Angeles, California – generated more than its fair share of awesome images. See photos.

Allan Der sent in this photo from Downey, California, on October 7, 2018: “SpaceX Falcon 9 first stage rocket. I was not expecting to shoot the event, but happen to have my camera handy.”

See it! Images of comet 46P/Wirtanen: Look here for photos and video of 2018’s Christmas comet and brightest comet 46P/Wirtanen. See photos.

Comet 46P/Wirtanen on December 15, 2018 – hours before it came closest to Earth – via Juan Gonzalez-Alicea in Cabo Rojo, Puerto Rico.

EarthSky 2019 lunar calendars are cool! Order now. Going fast!

Bottom line: Most popular EarthSky photos from 2018.



from EarthSky http://bit.ly/2Ais4aV

Northern Cross upright in west now

Tonight, look for the Northern Cross. It isn’t as famous as its counterpart – the Southern Cross – visible from the Southern Hemisphere or the northern tropics. But the Northern Cross also looks like a cross, and it’s pretty easy to spot. It’s a large, noticeable star pattern.

The star Deneb marks the top of the Northern Cross, and the star Albireo marks the bottom. Tonight you can find the Northern Cross shining fairly high in the west at nightfall, as seen from mid-northern latitudes. It sinks downward during the evening hours, and stands proudly over the west-northwest horizon around mid-evening.

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The Northern Cross, a clipped version of the constellation Cygnus the Swan. Photo credit: Janne

Here’s another look at the famous Northern Cross. It’s part of the constellation Cygnus the Swan. Photo via Flickr user Janne.

The Northern Cross is what’s known as an asterism. In other words, it’s not a constellation but simply a noticeable pattern of stars. It’s part of the constellation Cygnus the Swan.

As an added bonus, if you have a pair of binoculars, break them out this evening and point them toward the Northern Cross and its larger constellation Cygnus the Swan. In this direction, you’ll find a part of our Milky Way galaxy that is called the Cygnus Star Cloud. It is part of the spiral arm of our galaxy that also contains our sun, and you should be able to pick out stars from it if the night is clear in your area.

By the way, we get many questions from people in northern latitudes about if and when they can view the Southern Cross in their portion of the sky. The truth is that unless you live close to the tropics (Hawaii, or the southernmost parts of Texas or Florida for those of us in the U.S.), you will not be able to view the Southern Cross, also known as the constellation Crux. To find out how to locate Crux in Hawaii at this time of year, look here.

Bottom line: Learn to recognize a famous star pattern known as the Northern Cross, which stands upright over the west-northwest horizon in December.

Looking for a sky almanac? EarthSky recommends…

EarthSky lunar calendars make great gifts for astronomy-minded friends and family.



from EarthSky http://bit.ly/2Q4q3ny

Tonight, look for the Northern Cross. It isn’t as famous as its counterpart – the Southern Cross – visible from the Southern Hemisphere or the northern tropics. But the Northern Cross also looks like a cross, and it’s pretty easy to spot. It’s a large, noticeable star pattern.

The star Deneb marks the top of the Northern Cross, and the star Albireo marks the bottom. Tonight you can find the Northern Cross shining fairly high in the west at nightfall, as seen from mid-northern latitudes. It sinks downward during the evening hours, and stands proudly over the west-northwest horizon around mid-evening.

Donate: Your support means the world to us

The Northern Cross, a clipped version of the constellation Cygnus the Swan. Photo credit: Janne

Here’s another look at the famous Northern Cross. It’s part of the constellation Cygnus the Swan. Photo via Flickr user Janne.

The Northern Cross is what’s known as an asterism. In other words, it’s not a constellation but simply a noticeable pattern of stars. It’s part of the constellation Cygnus the Swan.

As an added bonus, if you have a pair of binoculars, break them out this evening and point them toward the Northern Cross and its larger constellation Cygnus the Swan. In this direction, you’ll find a part of our Milky Way galaxy that is called the Cygnus Star Cloud. It is part of the spiral arm of our galaxy that also contains our sun, and you should be able to pick out stars from it if the night is clear in your area.

By the way, we get many questions from people in northern latitudes about if and when they can view the Southern Cross in their portion of the sky. The truth is that unless you live close to the tropics (Hawaii, or the southernmost parts of Texas or Florida for those of us in the U.S.), you will not be able to view the Southern Cross, also known as the constellation Crux. To find out how to locate Crux in Hawaii at this time of year, look here.

Bottom line: Learn to recognize a famous star pattern known as the Northern Cross, which stands upright over the west-northwest horizon in December.

Looking for a sky almanac? EarthSky recommends…

EarthSky lunar calendars make great gifts for astronomy-minded friends and family.



from EarthSky http://bit.ly/2Q4q3ny

Global warming ‘hiatus’ is the climate change myth that refuses to die

Kevin Cowtan, Professor of Chemistry, University of York and Stephan Lewandowsky, Chair of Cognitive Psychology, University of Bristol

This article is republished from The Conversation under a Creative Commons license. Read the original article.

The record-breaking, El Niño-driven global temperatures of 2016 have given climate change deniers a new trope. Why, they ask, hasn’t it since got even hotter?

In response to a recent US government report on the impact of climate change, a spokesperson for the science-denying American Enterprise Institute think-tank claimed that “we just had […] the biggest drop in global temperatures that we have had since the 1980s, the biggest in the last 100 years.”

These claims are blatantly false: the past two years were two of the three hottest on record, and the drop in temperature from 2016 to 2018 was less than, say, the drop from 1998 (a previous record hot year) to 2000. But, more importantly, these claims use the same kind of misdirection as was used a few years ago about a supposed “pause” in warming lasting from roughly 1998 to 2013.

At the time, the alleged pause was cited by many people sceptical about the science of climate change as a reason not to act to reduce greenhouse pollution. US senator and former presidential candidate Ted Cruz frequently argued that this lack of warming undermined dire predictions by scientists about where we’re heading.

However, drawing conclusions on short-term trends is ill-advised because what matters to climate change is the decade-to-decade increase in temperatures rather than fluctuations in warming rate over a few years. Indeed, if short periods were suitable for drawing strong conclusions, climate scientists should perhaps now be talking about a “surge” in global warming since 2011, as shown in this figure:

Global temperature observations compared to climate models. Climate-disrupting volcanoes are shown at the bottom, and the purported hiatus period is shaded. 2018 values based on year to date (YTD). NASA; Berkeley Earth; various climate models., Author provided

The “pause” or “hiatus” in warming of the early 21st century is not just a talking point of think-tanks with radical political agendas. It also features in the scientific literature, including in the most recent report of the Intergovernmental Panel on Climate Change and more than 200 peer-reviewed articles.

Research we recently published in Environmental Research Letters addresses two questions about the putative “pause”: first, is there compelling evidence in the temperature data alone of something unusual happening at the start of the 21st century? Second, did the rise in temperature lag behind projections by climate models?

In both cases the answer is “no”, but the reasons are interesting.

Reconstructing a historical temperature record from instruments designed for other purposes, such as weather forecasting, is not always easy. Several problems have affected temperature estimates for the period since 2000. The first of these was the fact that uneven geographical distribution of weather stations can influence the apparent rate of warming. Other factors include changes in the instruments used to measure ocean temperatures. Most of these factors were known at the time and reported in the scientific literature, but because the magnitudes of the effects were unknown, users of temperature data (from science journalists to IPCC authors) were in a bind when interpreting their results.

‘This glacier was here in 1908’: warming might fluctuate, but the long-term trend is clear. Matty Symons/Shutterstock

A more subtle problem arises when we ask whether a fluctuation in the rate of warming is a new phenomena, rather than the kind of variation we expect due to natural fluctuations of the climate system. Different statistical tests are needed to determine whether a phenomena is interesting depending on how the data are chosen. In a nutshell, if you select data based on them being unusual in the first place, then any statistical tests that seemingly confirm their unusual nature give the wrong answer. (The statistical issue here is similar to the fascinating but counterintuitive “Monty Hall problem”, which has caught out many mathematicians).

When the statistical test is applied correctly, the apparent slowdown in warming is no more significant than other fluctuations in the rate of warming over the past 40 years. In other words, there is no compelling evidence that the supposed “pause” period is different from other previous periods. Neither is the deviation between the observations and climate model projections larger than would be expected.

That’s not to say that such “wiggles” in the temperature record are uninteresting – several of our team are involved in further studies of these fluctuations, and the study of the “pause” has yielded interesting new insights into the climate system – for example, the role of changes in the Atlantic and Pacific oceans.

There are lessons here for the media, for the public, and for scientists.

For scientists, there are two lessons: first, when you get to know a dataset by using it repeatedly in your work, make sure you also still remember the limitations you read about when first downloading it. Second, remember that your statistical choices are always part of a cascade of decisions, and at least occasionally those decisions must be revisited.

For the public and the media, the lesson is to check claims about the data. In particular, when claims are made based on short periods or specific datasets, they are often designed to mislead. If someone claims the world hasn’t warmed since 1998 or 2016, ask them why those specific years – why not 1997 or 2014? Why have such short limits at all? And also check how reliable similar claims have been in the past.

The technique of misinformation is nicely described in a quote attributed to climate researcher Michael Tobis:

“If a large data set speaks convincingly against you, find a smaller and noisier one that you can huffily cite.”

Global warming didn’t stop in 1998. Don’t be fooled by claims that it stopped in 2016 either. There is only one thing that will stop global warming: cuts to greenhouse gas emissions.



from Skeptical Science http://bit.ly/2SntQi7

Kevin Cowtan, Professor of Chemistry, University of York and Stephan Lewandowsky, Chair of Cognitive Psychology, University of Bristol

This article is republished from The Conversation under a Creative Commons license. Read the original article.

The record-breaking, El Niño-driven global temperatures of 2016 have given climate change deniers a new trope. Why, they ask, hasn’t it since got even hotter?

In response to a recent US government report on the impact of climate change, a spokesperson for the science-denying American Enterprise Institute think-tank claimed that “we just had […] the biggest drop in global temperatures that we have had since the 1980s, the biggest in the last 100 years.”

These claims are blatantly false: the past two years were two of the three hottest on record, and the drop in temperature from 2016 to 2018 was less than, say, the drop from 1998 (a previous record hot year) to 2000. But, more importantly, these claims use the same kind of misdirection as was used a few years ago about a supposed “pause” in warming lasting from roughly 1998 to 2013.

At the time, the alleged pause was cited by many people sceptical about the science of climate change as a reason not to act to reduce greenhouse pollution. US senator and former presidential candidate Ted Cruz frequently argued that this lack of warming undermined dire predictions by scientists about where we’re heading.

However, drawing conclusions on short-term trends is ill-advised because what matters to climate change is the decade-to-decade increase in temperatures rather than fluctuations in warming rate over a few years. Indeed, if short periods were suitable for drawing strong conclusions, climate scientists should perhaps now be talking about a “surge” in global warming since 2011, as shown in this figure:

Global temperature observations compared to climate models. Climate-disrupting volcanoes are shown at the bottom, and the purported hiatus period is shaded. 2018 values based on year to date (YTD). NASA; Berkeley Earth; various climate models., Author provided

The “pause” or “hiatus” in warming of the early 21st century is not just a talking point of think-tanks with radical political agendas. It also features in the scientific literature, including in the most recent report of the Intergovernmental Panel on Climate Change and more than 200 peer-reviewed articles.

Research we recently published in Environmental Research Letters addresses two questions about the putative “pause”: first, is there compelling evidence in the temperature data alone of something unusual happening at the start of the 21st century? Second, did the rise in temperature lag behind projections by climate models?

In both cases the answer is “no”, but the reasons are interesting.

Reconstructing a historical temperature record from instruments designed for other purposes, such as weather forecasting, is not always easy. Several problems have affected temperature estimates for the period since 2000. The first of these was the fact that uneven geographical distribution of weather stations can influence the apparent rate of warming. Other factors include changes in the instruments used to measure ocean temperatures. Most of these factors were known at the time and reported in the scientific literature, but because the magnitudes of the effects were unknown, users of temperature data (from science journalists to IPCC authors) were in a bind when interpreting their results.

‘This glacier was here in 1908’: warming might fluctuate, but the long-term trend is clear. Matty Symons/Shutterstock

A more subtle problem arises when we ask whether a fluctuation in the rate of warming is a new phenomena, rather than the kind of variation we expect due to natural fluctuations of the climate system. Different statistical tests are needed to determine whether a phenomena is interesting depending on how the data are chosen. In a nutshell, if you select data based on them being unusual in the first place, then any statistical tests that seemingly confirm their unusual nature give the wrong answer. (The statistical issue here is similar to the fascinating but counterintuitive “Monty Hall problem”, which has caught out many mathematicians).

When the statistical test is applied correctly, the apparent slowdown in warming is no more significant than other fluctuations in the rate of warming over the past 40 years. In other words, there is no compelling evidence that the supposed “pause” period is different from other previous periods. Neither is the deviation between the observations and climate model projections larger than would be expected.

That’s not to say that such “wiggles” in the temperature record are uninteresting – several of our team are involved in further studies of these fluctuations, and the study of the “pause” has yielded interesting new insights into the climate system – for example, the role of changes in the Atlantic and Pacific oceans.

There are lessons here for the media, for the public, and for scientists.

For scientists, there are two lessons: first, when you get to know a dataset by using it repeatedly in your work, make sure you also still remember the limitations you read about when first downloading it. Second, remember that your statistical choices are always part of a cascade of decisions, and at least occasionally those decisions must be revisited.

For the public and the media, the lesson is to check claims about the data. In particular, when claims are made based on short periods or specific datasets, they are often designed to mislead. If someone claims the world hasn’t warmed since 1998 or 2016, ask them why those specific years – why not 1997 or 2014? Why have such short limits at all? And also check how reliable similar claims have been in the past.

The technique of misinformation is nicely described in a quote attributed to climate researcher Michael Tobis:

“If a large data set speaks convincingly against you, find a smaller and noisier one that you can huffily cite.”

Global warming didn’t stop in 1998. Don’t be fooled by claims that it stopped in 2016 either. There is only one thing that will stop global warming: cuts to greenhouse gas emissions.



from Skeptical Science http://bit.ly/2SntQi7