Friday, November 22, 2013

Astrophoto: Plane Pwns the Moon

Astrophoto: Plane Pwns the Moon:
An airplane at about 2,400 meters above the ground  passes in front of the Moon on its way to landing at the Charles de Gaulle Airport in Paris, France. Taken from about 70 km from Paris. Credit and copyright: Sebastien Lebrigand.
Astrophoto: Plane Pwns the Moon
An airplane at about 2,400 meters above the ground passes in front of the Moon on its way to landing at the Charles de Gaulle Airport in Paris, France. Taken from about 70 km from Paris. Credit and copyright: Sebastien Lebrigand.
Astrophotgrapher Sebastien Lebrigand lives along the flight path to the Charles de Gaulle Airport in Paris and regularly captures planes flying in front of the Moon (see another of his shots here). But this might be the image to end all ‘plane crosses in front of the Moon’ pictures. This plane is seriously taking over the Moon! Plus, its a great detailed shot of the lunar surface.
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Astronomers Catch a Galactic Threesome in the Act

Astronomers Catch a Galactic Threesome in the Act:
A combined image from the Spitzer, Hubble, and Subaru telescopes show this structure to be three galaxies merging into one (NASA/JPL-Caltech/STScI/NAOJ/Subaru)
Astronomers Catch a Galactic Threesome in the Act
A combined image from the Spitzer, Hubble, and Subaru telescopes show this structure to be three galaxies merging into one (NASA/JPL-Caltech/STScI/NAOJ/Subaru)
An enormous and incredibly luminous distant galaxy has turned out to actually be three galaxies in the process of merging together, based on the latest observations from ALMA as well as the Hubble and Spitzer space telescopes. Located 13 billion light-years away, this galactic threesome is being seen near the very beginning of what astronomers call the “Cosmic Dawn,” a time when the Universe first became illuminated by stars.
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Thursday, November 21, 2013

Best Evidence Yet for a High-Energy Jet Emanating from the Milky Way’s Black Hole

Best Evidence Yet for a High-Energy Jet Emanating from the Milky Way’s Black Hole:
A composite image in X-ray and radio showing a likely candidate for a jet emanating from the supermassive black hole at the center of the Milky Way. X-ray: NASA/CXC/UCLA/Z.Li et al; Radio: NRAO/VLA
Best Evidence Yet for a High-Energy Jet Emanating from the Milky Way’s Black Hole
A composite image in X-ray and radio showing a likely candidate for a jet emanating from the supermassive black hole at the center of the Milky Way. X-ray: NASA/CXC/UCLA/Z.Li et al; Radio: NRAO/VLA
Jets of high energy particles emanating from a black hole have been detected plenty of times before, but in other galaxies, that is — not from the supermassive black hole at the center of the Milky Way, known as Sagittarius A* (Sgr A*). Previous studies and other evidence suggested that perhaps there were jets – or ghosts of past jets – but many findings and studies often contradicted each other, and none were considered definitive.
Now, astronomers using Chandra X-ray Observatory and the Very Large Array (VLA) radio telescope have found strong evidence Sgr A* is producing a jet of high-energy particles.
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Wednesday, November 20, 2013

Asteroids Can Get Shaken And Stirred By Mars’ Gravity

Asteroids Can Get Shaken And Stirred By Mars’ Gravity:
Artist's conception of Mars, with asteroids nearby. Credit: NASA
Asteroids Can Get Shaken And Stirred By Mars’ Gravity
Artist’s conception of Mars, with asteroids nearby. Credit: NASA
Asteroids are sometimes called loose rubble piles, which leads to interesting effects if they happen to get close to a planet. A science team in 2010 found out that when asteroids get close to Earth, the gravity of our planet can stir up the dust grains and “refresh” its face, in a sense. Now, scientists have found that Mars can do the same thing.
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Exploring Our Galaxy’s Ancient Brown Dwarfs

Exploring Our Galaxy’s Ancient Brown Dwarfs:
A brown dwarf from the thick-disk or halo is shown. Although astronomers observe these objects as they pass near to the solar system, they spend much of their time away from the busiest part of the Galaxy, and the Milky Way's disk can be seen in the background. Credit: John Pinfield
Exploring Our Galaxy’s Ancient Brown Dwarfs
A brown dwarf from the thick-disk or halo is shown. Although astronomers observe these objects as they pass near to the solar system, they spend much of their time away from the busiest part of the Galaxy, and the Milky Way’s disk can be seen in the background. Credit: John Pinfield
As the name implies, a brown dwarf is small… only about 7% the size of the Sun. As far as stellar senior citizens go, they’re cool. Zipping along through space at speeds of 100 to 200 kilometers per second, they may have formed back when our galaxy was young – perhaps 10 billion years ago. Now a team of astronomers headed by Dr. David Pinfield at the University of Hertfordshire has identified a pair of the oldest brown dwarfs known… a set of orbs which could be the harbinger of a huge amount of new, unseen objects. (...)
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Tuesday, November 19, 2013

A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group

A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group:
NGC 5044 as seen in a composite image from the Wide-field Infrared Survey Explorer, the Digitized Sky Survey (optical), Galex (near-ultraviolet) and new X-ray observations from XMM-Newton (in blue.) Astronomers say they are able to see hot gas moving in this galaxy because of an interaction with another galaxy millions of years ago. Credit: E. O’Sullivan & ESA
A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group
NGC 5044 as seen in a composite image from the Wide-field Infrared Survey Explorer, the Digitized Sky Survey (optical), Galex (near-ultraviolet) and new X-ray observations from XMM-Newton (in blue.) Astronomers say they are able to see hot gas moving in this galaxy because of an interaction with another galaxy millions of years ago. Credit: E. O’Sullivan & ESA
So galaxy group NGC 5044 was just sitting quietly by itself a few million years ago when galaxy NGC 5054 decided to pass right through it. That close encounter finished long ago, but the ricochet is still visible in telescopes as astronomers spotted hot gas rippling through the host galaxy.
(...)
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‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation

‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation:
NGC 3572 seen with a 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile. Credit: ESO/G. Beccari
‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation
NGC 3572 seen with a 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile. Credit: ESO/G. Beccari
Star winds are pushing the gas around NGC 3572 into “elephant trunks”, as you can see if you look carefully as this picture snapped by a La Silla Observatory telescope at the European Southern Observatory in Chile. It’s a demonstration of the power of the youngster blue-white stars embedded in the cloud, which are generating huge gusts blowing the gas and dust away from them.
It’s common for young stars to form in groups. After a few million years growing together, their respective gravities pushes everything further apart, and the stars then finish their lifetimes on their own. Looking at young star clusters such as this gives astronomers a better sense about how our own Sun began its life.
If we zoomed closer to those elephant trunks, they would look similar to the famous “Pillars of Creation” image captured in 1995 by the Hubble Space Telescope in the Eagle Nebula (M16). NASA also did a follow-up observation using infrared wavelengths in 2005 and 2011, which made the young stars a bit easier to see amid the gas and dust.
(...)
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UrtheCast: Cameras for Live Video Views of Planet Earth To Launch Nov. 25

UrtheCast: Cameras for Live Video Views of Planet Earth To Launch Nov. 25:
A view of rivers in Montana, USA, from the ISS. Credit: ESA/Luca Parmitano.
UrtheCast: Cameras for Live Video Views of Planet Earth To Launch Nov. 25
A view of rivers in Montana, USA, from the ISS. Credit: ESA/Luca Parmitano.
A Canadian camera system aiming to provide near-realtime video views of Earth is readying for a launch from Kazakhstan.
If all goes well, the UrtheCast dual camera system will blast off in a Progress supply ship on Nov. 25, 2013.
This will be the world’s first ever high definition, live-streaming video platform of planet Earth from the International Space Station.
(...)
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Teenaged Space Station Thriving After 15 Years Of Science, Extreme Construction And Tricky Repairs

Teenaged Space Station Thriving After 15 Years Of Science, Extreme Construction And Tricky Repairs:
The International Space Station in March 2009 as seen from the departing STS-119 space shuttle Discovery crew. Credit: NASA/ESA
Teenaged Space Station Thriving After 15 Years Of Science, Extreme Construction And Tricky Repairs
The International Space Station in March 2009 as seen from the departing STS-119 space shuttle Discovery crew. Credit: NASA/ESA
Extreme conditions surround the International Space Station’s scientific work, to say the least. It takes a rocketship to get there. Construction required more than 1,000 hours of people using spacesuits. Astronauts must balance their scientific work with the need to repair stuff when it breaks (like an ammonia coolant leak this past spring.)
But amid these conditions, despite what could have been show-stoppers to construction such as the Columbia shuttle tragedy of 2003, and in the face of changing political priorities and funding from the many nations building the station, there the ISS orbits. Fully built, although more is being added every year. The first module (Zarya) launched into space 15 years ago tomorrow. Humans have been on board continuously since November 2000, an incredible 13 years.
The bulk of construction wrapped up in 2011, but the station is still growing and changing and producing science for the researchers sending experiments up there. Below are some of the milestones of construction in the past couple of decades. Did we miss something important? Let us know in the comments.
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Using the ‘Missing Physics’ of Stellar Feedback to Accurately Simulate Galaxies from the Big Bang to Today

Using the ‘Missing Physics’ of Stellar Feedback to Accurately Simulate Galaxies from the Big Bang to Today:
A simulated dwarf galaxy when the universe was 0.5 billion years old. Magenta represents cool gas, green is warm ionized gas, and red is hot gas. Check out the movie. Image credit: Hopkins et al. 2013.
Using the ‘Missing Physics’ of Stellar Feedback to Accurately Simulate Galaxies from the Big Bang to Today
A simulated dwarf galaxy when the universe was 0.5 billion years old. Magenta represents cool gas, green is warm ionized gas, and red is hot gas. Check out the movie by clicking above. Image credit: Hopkins et al. 2013.
For the first time, astronomers are able to accurately simulate galaxies from shortly after the big bang to today by including a realistic treatment of the effects stars have on their host galaxies.
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Monday, November 18, 2013

A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group

A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group:
NGC 5044 as seen in a composite image from the Wide-field Infrared Survey Explorer, the Digitized Sky Survey (optical), Galex (near-ultraviolet) and new X-ray observations from XMM-Newton (in blue.) Astronomers say they are able to see hot gas moving in this galaxy because of an interaction with another galaxy millions of years ago. Credit: E. O’Sullivan & ESA
A Cosmic Intruder Grabbed Hot Gas From This Galaxy Group
NGC 5044 as seen in a composite image from the Wide-field Infrared Survey Explorer, the Digitized Sky Survey (optical), Galex (near-ultraviolet) and new X-ray observations from XMM-Newton (in blue.) Astronomers say they are able to see hot gas moving in this galaxy because of an interaction with another galaxy millions of years ago. Credit: E. O’Sullivan & ESA
So galaxy group NGC 5044 was just sitting quietly by itself a few million years ago when galaxy NGC 5054 decided to pass right through it. That close encounter finished long ago, but the ricochet is still visible in telescopes as astronomers spotted hot gas rippling through the host galaxy.
(...)
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‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation

‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation:
NGC 3572 seen with a 2.2-meter telescope at the European Southern Observatory's La Silla Observatory in Chile. Credit: ESO/G. Beccari
‘Elephant Trunks’ Crowd Distant Star Cluster, Raising New Questions About Stellar Formation
NGC 3572 seen with a 2.2-meter telescope at the European Southern Observatory’s La Silla Observatory in Chile. Credit: ESO/G. Beccari
Star winds are pushing the gas around NGC 3572 into “elephant trunks”, as you can see if you look carefully as this picture snapped by a La Silla Observatory telescope at the European Southern Observatory in Chile. It’s a demonstration of the power of the youngster blue-white stars embedded in the cloud, which are generating huge gusts blowing the gas and dust away from them.
It’s common for young stars to form in groups. After a few million years growing together, their respective gravities pushes everything further apart, and the stars then finish their lifetimes on their own. Looking at young star clusters such as this gives astronomers a better sense about how our own Sun began its life.
If we zoomed closer to those elephant trunks, they would look similar to the famous “Pillars of Creation” image captured in 1995 by the Hubble Space Telescope in the Eagle Nebula (M16). NASA also did a follow-up observation using infrared wavelengths in 2005 and 2011, which made the young stars a bit easier to see amid the gas and dust.
(...)
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European satellite burns up after plunging into Earth’s atmosphere

European satellite burns up after plunging into Earth’s atmosphere:
True colour satellite image of the Earth centred on Asia and Oceania with cloud coverage, during summer solstice at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites., Globe Centred On Asia And Oceania, True Colour Satellite Image (Photo by Planet Observer/Universal Images Group via Getty Images)
European satellite burns up after plunging into Earth’s atmosphere
True colour satellite image of the Earth centred on Asia and Oceania with cloud coverage, during summer solstice at 6 a.m GMT. This image in orthographic projection was compiled from data acquired by LANDSAT 5 & 7 satellites., Globe Centred On Asia And Oceania. Credit: Getty Images
A 1-ton European science satellite plunged back into Earth’s atmosphere and incinerated with debris most likely landing in the southern regions of the Atlantic Ocean, officials said on Monday.
The last contact by ground tracking stations with Europe’s Gravity field and steady-state Ocean Circulation Explorer, known as GOCE, was at 5:42 p.m. EST  on Sunday as the spacecraft flew just 75 miles above Antarctica, the European Space Agency said.
Extrapolating from computer models, officials believe GOCE hit the upper atmosphere about 50 miles above the planet’s surface no later than 7:16 p.m. EST Sunday near the Falkland Islands.
“This would put the main area over which any possible GOCE remnants fell to the southernmost regions of the Atlantic Ocean,” the space agency wrote in a status report on its website.
“No damage to property has been reported from any debris,” the report said.
About 25 percent of the car-sized satellite was expected to have survived re-entry.
GOCE was launched in 2009 to map variations in Earth’s gravity. Scientists assembled the data into the first detailed global maps of the boundary between the planet’s crust and mantle, among other projects.
The satellite ran out of fuel on Oct. 21 and had been steadily losing altitude since, tugged by Earth’s gravity.
The 1.2-ton GOCE satellite is small in comparison to other spacecraft that recently crashed back into the atmosphere.
In January 2012, Russia’s failed 14-ton Phobos-Grunt Mars probe returned. In 2011, NASA’s 6.5-ton Upper Atmosphere Research Satellite and Germany’s 2.4-ton  X-ray ROSAT telescope re-entered the atmosphere.

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Friday, November 15, 2013

Delving Into The Mystery Of Black Hole Jets

Delving Into The Mystery Of Black Hole Jets:
Black hole with disc and jets visualization courtesy of ESA
Delving Into The Mystery Of Black Hole Jets
Black hole with disc and jets visualization courtesy of ESA
The concept of a black hole jet isn’t a new one, but we still have a lot to learn about the mixture of particles found in the vacinity of them. Through the use of ESA’s XMM-Newton Observatory, astronomers have been taking a look at a black hole in our galaxy and found some surprising results. (...)
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Comet ISON Suddenly Brightens as it Dives Toward the Sun

Comet ISON Suddenly Brightens as it Dives Toward the Sun:
Mike Hankey of Monkton, Maryland took this photo of Comet ISON in outburst this morning Nov. 14. The tail now shows multiple streamers. Click to enlarge. Credit: Mike Hankey
Comet ISON Suddenly Brightens as it Dives Toward the Sun
Mike Hankey of Monkton, Maryland took this photo of Comet ISON in outburst this morning Nov. 14. The tail now shows multiple streamers. Click to enlarge. Credit: Mike Hankey
After a sleepy week, Comet ISON is suddenly coming alive. Several amateur astronomers and at least one professional astronomers are reporting today that the comet has brightened at least a full magnitude overnight.  Two days ago it glowed at around magnitude 7.5 and was visible weakly in 10×50 binoculars from a dark sky. Now it’s surged to around magnitude 6 – naked eye limit – and continues to brighten. ISON’s appearance has radically changed too.
(...)
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How Astronauts Can Explore The Martian Moon Phobos

How Astronauts Can Explore The Martian Moon Phobos:
Projected timeline of the MARS-X project. Credit: MARS-X
How Astronauts Can Explore The Martian Moon Phobos
Projected timeline of the MARS-X project. Credit: MARS-X
OTTAWA, CANADA – Humans would spend more than a year orbiting and bouncing on the Martian moon Phobos under a mission concept developed by students at the International Space University.
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Astrophotos: Aurora Reflections from Iceland

Astrophotos: Aurora Reflections from Iceland:
Aurora Borealis, beach reflection, and Orion, in Iceland on the beach Jökulsarlon. Image was taken on November 7, 2013. Credit and copyright Cory Schmitz
Astrophotos: Aurora Reflections from Iceland
Aurora Borealis, beach reflection, and Orion, in Iceland on the beach Jökulsarlon. Image was taken on November 7, 2013. Credit and copyright Cory Schmitz
Our friend Cory Schmitz planned the perfect time to go on a Iceland Aurora photo tour. With the recent activity from the Sun, there have been some great views of the aurora borealis in Iceland. “These images are very close to what the sky actually looked like to the naked eye,” Cory said on G+. “Motion, color, everything. Right above our heads. Insane — what an experience!”
Thanks for sharing the experience, Cory…. but next time, bring us with you, huh?
(...)
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Wednesday, November 13, 2013

Sgr A* Could Be a Relic of a Powerful AGN

Sgr A* Could Be a Relic of a Powerful AGN:
The Magellanic Stream
Sgr A* Could Be a Relic of a Powerful AGN
The Magellanic Stream as imaged by the Hubble Space Telescope. Note the red color. Image Credit: NASA.
The early universe was sizzling with active galactic nuclei (AGN) — intensely luminous cores powered by supermassive black holes — most of which could outshine their entire host galaxies and be seen across the observable universe.
While our central supermassive black hole Sgr A* lies rather dormant at the moment, new evidence suggests that it too was once a powerful AGN.
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Moon’s Blotchy Near Side Has Bigger Craters Than Expected

Moon’s Blotchy Near Side Has Bigger Craters Than Expected:
The thickness of the moon's crust as calculated by NASA's GRAIL mission. The near side is on the left-hand side of the picture, and the far side on the right. Credit: NASA/JPL-Caltech/S. Miljkovic
Moon’s Blotchy Near Side Has Bigger Craters Than Expected
The thickness of the moon’s crust as calculated by NASA’s GRAIL mission. The near side is on the left-hand side of the picture, and the far side on the right. Credit: NASA/JPL-Caltech/S. Miljkovic
The familiar blotches that make up “the man in the moon”, from the vantage point of Earth, happened because the moon’s crust is thinner on the near side than the far side to our planet, new research reveals.
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Astronomy Cast 321: Solar Flares

Astronomy Cast 321: Solar Flares:


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Track Comet ISON’s Journey Around the Sun with this Paper Model

Track Comet ISON’s Journey Around the Sun with this Paper Model:
Comet ISON is making its way through the inner solar system. Visualize its unusual orbit and track its journey  around the sun with this paper model. The background image shows comet  C/2001 Q4 (NEAT). Credit: NASA and T. A. Rector (Univ. of Alaska Anchorage), Z. Levay and L. Frattare (STScI) and WIYN/NOAO/AURA/NSF
Track Comet ISON’s Journey Around the Sun with this Paper Model
As Comet ISON loops around the sun and back, you can visualize its unusual orbit and track its progress with this paper model. The background image shows comet C/2001 Q4 (NEAT). Credit: NASA and T. A. Rector, Z. Levay and L. Frattare and WIYN/NOAO/AURA/NSF
Planet orbits are so easy to picture – eight nearly concentric hula hoops centered on the sun. Comets are weirder. Their orbits vary from tapered ellipses shaped like cigars to completely open-ended parabolas and even hyperbolas. Comet ISON’s highly-elongated (stretched out) orbit is best described as hyperbolic, although that’s subject to change if Jupiter gets into the act and gives the comet a gravitational nudge during its outbound journey. As the largest planet, it has a special knack for this kind of trick, having tamed many a wayward comet’s orbit into a neat ellipse.
(...)
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Space Internet? Rocket Flight Aims To Test Earth-To-Space Communications

Space Internet? Rocket Flight Aims To Test Earth-To-Space Communications:
The cameras mounted in the ISS's cupola could serve as the platform for the first-ever quantum optics experiment in space.
Space Internet? Rocket Flight Aims To Test Earth-To-Space Communications
Earth from the International Space Station’s Cupola window. Credit: NASA
Imagine you’re a space tourist wanting to blog about your experience. Too impatient to wait for the ride back to solid ground, you open up your laptop on the way home and post pictures and video of the experience just minutes after you were zooming through suborbital space.
That would only be possible if there was some sort of infrastructure available to send messages over the Internet or on text protocols, and according to Brian Barnett, there’s plenty of demand from the private sector, NASA and universities to do so. That’s why this morning, his company (Satwest) will put a temporary wi-fi hotspot in space aboard a rocket from Denver’s UP Aerospace Inc.
(...)
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Supersonic Starbirth Bubble Glows In Image From Two Telescopes

Supersonic Starbirth Bubble Glows In Image From Two Telescopes:
Stellar birth is visible in this image of HH 46/47 taken with the Spitzer Space Telescope and Atacama Large Millimeter/submillimeter Array (ALMA). Credit: NASA/JPL-Caltech/ALMA
Supersonic Starbirth Bubble Glows In Image From Two Telescopes
Stellar birth is visible in this image of HH 46/47 taken with the Spitzer Space Telescope and Atacama Large Millimeter/submillimeter Array (ALMA). Credit: NASA/JPL-Caltech/ALMA
Talk about birth in the fast lane. Fresh observations of HH 46/47 — an area well-known for hosting a baby star — demonstrate material from the star pushing against the surrounding gas at supersonic speeds.
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