Grus

Grus

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The constellation of Grus was originally created by Petrus Plancius from the observations of Dutch sea navigators Pieter Dirkszoon Keyser and Frederick de Houtman when exploring the southern hemisphere. Grus’ stellar patterns became known when it appeared on a celestial globe in 1597 and was considered a constellation when it was added to Johann Bayer’s Uranometria catalog in 1603. It survived the years to become one of the 88 modern constellations recognized by the International Astronomical Union. Grus is located south of the ecliptic plane and covers approximately 366 square degrees of sky. It is bordered by the constellations of Piscis Austrinus, Microscopium, Indus, Tucana, Phoenix and Sculptor. The asterism consists of 7 main stars and there are 28 stars with Bayer/Flamsteed designations. Grus is visible to all observers at latitudes between +34° and ?34° and is best seen at culmination during the month of October.

Until the late 16th century, Grus was considered part of Piscis Austrinus – the “Southern Fish” – since most of its stars weren’t visible to northern latitudes. When exploration began below the equator many wondrous new creatures were discovered. One such bird was the fishing crane – Phoenicopterus – the flamingo. Perhaps this is how the constellation got is name, since Grus is also Dutch for “crane”!

First let’s take a binocular tour of Grus, starting with its brightest star, Alpha, the “a” symbol on our map. Alpha Gruis proper name is Alnair, the Arabic word for “bright one of the tail”. In this case, it was originally the tail of the fish. But besides being a bit “fishy”, Alnair is a hot, blue subgiant giant star about 101 light years away from Earth. Not only is it larger, hotter and brighter than our own Sol, but it a rather fast stellar rotation – making a complete rotation in under a day. Hop on to Beta Gruis, the “B” symbol on our map. Beta Gruis is a rare kind of star – a cooler class M giant star. It is very possible it is in an advanced state of evolution, losing mass and brightening with a dead carbon-oxygen core in preparation for sloughing its outer envelope – ready to become a Cepheid variable!

Now for visual and binocular double star, Delta 1 and Delta 2 Gruis – the “8” symbol in the center of the constellation. While this pair aren’t physically connect to one another, they do make a pleasing sight with their lovely yellow and red contrasting colors. For a true telescopic binary star, hop north to Upsilon. This disparate pair is separated by over a degree of arc and the difference between stellar magnitudes is a great experience.

For the telescope, tackle NGC 7213 (RA 22:09.3 Dec -47:10) about 16′ southeast of Alpha. This 10th magnitude Seyfert galaxy has definitely got some stories to tell. Not only is it a spiral galaxy, but one that has an incredible,giant H-alpha filament erupting from its nucleus. Another great challenge is NGC 7582, 7590 and 7599 (RA 023:19 Dec -42:3). Here is a small galaxy group consisting of three faint spirals in the same field, all tilted close to edge on. While at least an intermediate sized telescope is need to see them, a wide field eyepiece will place all three in the same field of view at around 100x magnification. Before we leave for the night, let’s try NGC 7410 (22:55.0 -39:40). This uniformly illuminated tilted spiral galaxy shows little sign of structure, despite its bright nature.

Sources: Wikipedia, SEDS
Chart courtesy of Your Sky.

Deepest Ultraviolet Image Shows a Sea of Distant Galaxies

A Pool of Distant Galaxies. Credit: ESO

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Dive right in to this image that contains a sea of distant galaxies! The Very Large Telescope has obtained the deepest ground-based image in the ultraviolet band, and here, you can see this patch of the sky is almost completely covered by galaxies, each one, like our own Milky Way galaxy, and home of hundreds of billions of stars. A few notable things about this image: galaxies were detected that are a billion times fainter than the unaided eye can see, and also in colors not directly observable by the human eye. In this image, a large number of new galaxies were discovered that are so far away that they are seen as they were when the Universe was only 2 billion years old! Also…

This image contains more than 27 million pixels and is the result of 55 hours of observation, made primarily with the Visible Multi Object Spectrograph (VIMOS) instrument. To get the full glory of this image, here’s where you can download the full resolution version. It’s worth the wait while it downloads. Or click here to be able to zoom around the image.

In this sea of galaxies – or island universes as they are sometimes called – only a very few stars belonging to the Milky Way are seen. One of them is so close that it moves very fast on the sky. This “high proper motion star” is visible to the left of the second brightest star in the image. It appears as a funny elongated rainbow because the star moved while the data were being taken in the different filters over several years.

The VLT folks describe this image as a “uniquely beautiful patchwork image, with its myriad of brightly coloured galaxies.” It shows the Chandra Deep Field South (CDF-S), one of the most observed and best studied regions in the entire sky. The CDF-S is one of the two regions selected as part of the Great Observatories Origins Deep Survey (GOODS), an effort of the worldwide astronomical community that unites the deepest observations from ground- and space-based facilities at all wavelengths from X-ray to radio. Its primary purpose is to provide astronomers with the most sensitive census of the distant Universe to assist in their study of the formation and evolution of galaxies.

The image encompasses 40 hours of observations with the VLT, just staring at the same region of the sky. The VIMOS R-band image was obtained co-adding a large number of archival images totaling 15 hours of exposure.

Source: ESO

Weekend SkyWatcher’s Forecast – November 7-9, 2008

Greetings, fellow StarGeezers! It’s Friiiii day… And another great weekend forecast. Does having all this Moon around get you down? It shouldn’t. Where else could you find another world that you could so intimately study detail with even the most modest of telescopes or binoculars? Instead of cursing Luna’s presence, get out your optics and enjoy! While we’re at it, we’ll take a look at some very interesting stars – both in the sky and from planet Earth. It’s time to head out into the dark… Cuz’ here’s what’s up!

Friday, November 7, 2008 – Today in 1996, the Mars Global Surveyor left on its journey. Just 30 years beforehand on this same day, Lunar Orbiter 2 was launched. Tonight let’s launch our way toward the Moon as we begin our observing evening with a look at a far northern crater – J. Herschel.

Residing on the mid-northern edge of Mare Frigoris, this huge, shallow old crater spans 156 kilometers and bear the scars of the years. Look for the deeper and younger crater Horrebow on the southwestern wall – for it has obliterated another, older wall crater.

Ready to aim for a bullseye? Then follow the “Archer” and head right for the bright, reddish star Aldebaran. Set your eyes, scopes or binoculars there and let’s look into the “eye” of the Bull.

Known to the Arabs as Al Dabaran, or “the Follower,” Alpha Tauri got its name because it appears to follow the Pleiades across the sky. In Latin it was called Stella Dominatrix, yet the Olde English knew it as Oculus Tauri, or very literally the “eye of Taurus.” No matter which source of ancient astronomical lore we explore, there are references to Aldebaran.

As the 13th brightest star in the sky, it almost appears from Earth to be a member of the V-shaped Hyades star cluster, but this association is merely coincidental, since it is about twice as close to us as the cluster is. In reality, Aldebaran is on the small end as far as K5 stars go, and like many other orange giants, it could possibly be a variable. Aldebaran is also known to have five close companions, but they are faint and very difficult to observe with backyard equipment. At a distance of approximately 68 light-years, Alpha is “only” about 40 times larger than our own Sun and approximately 125 times brighter. To try to grasp such a size, think of it as being about the same size as Earth’s orbit! Because of its position along the ecliptic, Aldebaran is one of the very few stars of first magnitude that can be occulted by the Moon.

Saturday, November 8, 2008 – Even if you only use binoculars tonight, you can’t miss the beautiful C-shape of Sinus Iridum as it comes into view on the lunar surface. As we have learned, the mountains ringing it are called the Juras, and the crater punctuating them is named Bianchini. Do you remember what the bright tips of the opening into the “Bay of Rainbows” are called? That’s right: Promontorium LaPlace to the northeast and Promontorium Heraclides to the southwest. Now take a good look at Heraclides… Just south of here is where Luna 17 landed, leaving the Lunokhod rover to explore!

Born on this day in 1656, the great Edmund Halley made his mark on history as he became best known for determining the orbital period of the comet which bears his name. English scientist Halley had multiple talents however, and in 1718 discovered that what were then referred to as “fixed stars,” actually displayed (proper) motion! If it were not for Halley, Sir Isaac Newton may never have published his now famous work on the laws of gravity and motion.

Now turn your eyes or binoculars just west of bright Aldebaran and have a look at the Hyades Star Cluster. As noted yesterday, Aldebaran appears to be part of this large, V-shaped group, but is not an actual member. The Hyades cluster is one of the nearest galactic clusters, and it is roughly 130 light-years away at its center. This moving group of stars is drifting slowly away toward Orion, and in another 50 million years will require a telescope to view!

Sunday, November 9, 2008 – Today is the birth date of Carl Sagan. Born in 1934, Sagan was an American planetologist, exobiologist, popularizer of science and astronomy, and novelist. During his lifetime, Sagan published more than 600 scientific papers and popular articles and was author, co-author, or editor of more than 20 books. His influential work and enthusiasm inspired us all. As Dr. Sagan once said, “Personally, I would be delighted if there were a life after death, especially if it permitted me to continue to learn about this world and others, if it gave me a chance to discover how history turns out.”

May his dreams live on..

If Carl were with us tonight, he would encourage amateurs at every level of astronomical ability! So let us honor his memory by beginning with an optical pairing of stars known as Zeta and Chi Ceti, a little more than a fistwidth northeast of bright Beta. Now have a look with binoculars or small scopes because you’ll find that each has its own optical companion!

Now drop south-southwest less than a fistwidth to have a look at something so unusual that you can’t help but be charmed – the UV Ceti System (RA 01 39 01 Dec -17 57 01).

What exactly is it? Also known as L 726-8, you are looking at two of the smallest and faintest stars known. This dwarf red binary system is the sixth nearest star to our solar system and resides right around nine light-years away. While you are going to need at least an intermediate-size scope to pick up these near 13th magnitude points of light, don’t stop observing right after you locate it. The fainter member of the two is what is known as a “Luyten’s Flare Star” (hence the “L” in its name). Although it doesn’t have a predictable timetable, this seemingly uninteresting star can jump two magnitudes in less than 60 seconds and drop back to “normal” within minutes – the cycle repeating possibly two or three times every 24 hours. A most incredible incident was recorded in 1952 when UV jumped from magnitude 12.3 to 6.8 in just 20 seconds!

No matter what you choose to look at tonight, as Dr. Sagan would say: “We are all star stuff.”

Have a great week and I’ll see you… Under the stars!

This week’s awesome photos are: Crater J. Herschel – Credit: Wes Higgins, Aldebaran – Credit: Palomar Observatory, courtesy of Caltech, Sinus Iridum – Credit: Wes Higgins, Edmund Halley (widely used public image), The Hyades Star Cluster – Credit: NASA, Carl Sagan (widely used public image), and Chi and the UV Ceti System – Credit: Palomar Observatory, courtesy of Caltech. Our many thanks to you!

Are We Close to Finding Dark Matter?

Dark Matter Halo. Credit: Virgo Consortium

Scientists say he search for the mysterious substance which makes up most of the Universe could soon be at an end. A massive computer simulation was used to show the evolution of a galaxy like the Milky Way, and analysts were able to “see” gamma-rays given off by dark matter. Dark matter is believed to account for 85 per cent of the Universe’s mass but has remained invisible to telescopes since scientists inferred its existence from its gravitational effects more than 75 years ago. If the computations are correct, the findings could help NASA’s Fermi Telescope to search for the dark matter and open a new chapter in our understanding of the Universe.

The consortium of scientists, called Virgo Consortium looked at dark matter halos – structures surrounding galaxies – which contain a trillion times the mass of the Sun. The simulations showed how the galaxy’s halo grew through a series of violent collisions and mergers between much smaller clumps of dark matter that emerged from the Big Bang.

The researchers found that gamma-rays produced when particles collided in areas of high dark matter density could be most easily detectable in regions of the Milky Way lying close to the Sun in the general direction of the galaxy’s centre.

They suggest the Fermi Telescope should search in this part of the galaxy where they predict that gamma-rays from dark matter should glow in “a smoothly varying and characteristic pattern”.

If Fermi does detect the predicted emission from the Milky Way’s smooth inner halo the Virgo team believes it might be able to see otherwise invisible clumps of dark matter lying very close to the Sun.

The Virgo research involved scientists from the Max Planck Institute for Astrophysics in Germany, The Institute for Computational Cosmology at Durham University, UK, the University of Victoria in Canada, the University of Massachusetts, USA, and the University of Groningen in the Netherlands.

Professor Carlos Frenk, Director of the Institute for Computational Cosmology, at Durham University, said: “Solving the dark matter riddle will be one of the greatest scientific achievements of our time.

“The search for dark matter has dominated cosmology for many decades. It may soon come to an end.”

Sources: EurekAlert, Virgo Consortium

Floating Battle Droids On Board ISS

SPHERES on the ISS. Credit: NASA

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Three free-flying spheres are currently zooming around inside the International Space Station. Is the crew of Expedition 18 using them to hone their light-saber battle skills a la Luke Skywalker or sharpen their ability to detect UFOs? No, these bowling-ball sized spherical satellites are part of an experiment devised by students at the Massachusetts Institute of Technology (MIT) to test autonomous rendezvous and docking maneuvers for future formation flying spacecraft. Called SPHERES – which stands for Synchronized Position Hold, Engage, Reorient, Experimental Satellites — these color-coded robots are flying inside the ISS, testing different flight formations. But these have to be a lot of fun to play with during off hours on the space station: zero-g bowling or space volleyball, anyone?

Astronauts Greg Chamitoff, Mike Fincke and spaceflight participant Richard Garriott posed with SPHERES.  Credit: NASA
Astronauts Greg Chamitoff, Mike Fincke and spaceflight participant Richard Garriott posed with SPHERES. Credit: NASA

Each satellite is self-contained with power, propulsion, computers and navigation equipment. The results are important for satellite servicing, vehicle assembly and formation flying spacecraft configurations. One future formation flying mission is the Terrestrial Planet Finder Interferometer, which will use multiple small vehicles flying in formation to create an orbiting infrared interferometer.
Terrestrial Planet Finder Interferometer array.
Terrestrial Planet Finder Interferometer array.

If successful, these mini-satellites, and their potentially larger versions, would be able to refuel/repair other satellites, establish positioning around space-based telescopes, and support space docking routines. So, battle droids would become maintenance droids.

And smaller, multiple satellite missions are economical and provide redundancy. Instead of launching one big, heavy satellite, launching lots of little is easier. They can orbit Earth in tandem, each doing their own small part of the overall mission. If a solar flare zaps one satellite—no problem. The rest can close ranks and carry on. Launch costs are reduced, too, because tiny satellites can hitch a ride inside larger payloads, getting to space almost free of charge.

The SPHERES can also test the ability to build spaceships in orbit. One way to build a larger ship to go to, for instance, Mars, is to assemble it piece by piece in Earth orbit. The SPHERES are helping engineers design software that could be used to maneuver the pieces of a spaceship together.

Sources: Science@NASA, NASA, MIT

Chandrayaan-1 Closer to the Moon; Snaps First Lunar Shot

Artists impress of Chandrayaan-1 at the moon. Credit: ISRO

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Following the fifth and final orbit raising maneuver which put Chandrayaan-1 closer to the moon, the spacecraft snapped the first picture of its final destination. This clear, crisp image of the moon While the images are still being processed and are not available yet, mission managers says the images bode well for spacecraft’s mission to map the entire moon’s surface with its Terrain Mapping Camera. And all systems are go for the final maneuver on November 8, which will put Chandrayaan-1 in lunar orbit.

After launch on October 22, the spacecraft was first injected into an elliptical 7-hr orbit around Earth, at 255 km from Earth at perigee (its closest point) and 22,860 km away at apogee, its farthest point. After five engine firings, Chandrayaan-1 has spiraled outwards in increasingly elongated ellipses around Earth, until it reached its lunar transfer orbit on November 4.

Chandrayaan-1 in its lunar transfer orbit.  Credit: ISRO
Chandrayaan-1 in its lunar transfer orbit. Credit: ISRO

In the final maneuver, engineers fired the spacecraft’s 440 Newton liquid-fuel propelled engine for about two and a half minutes. The lunar transfer orbit’s farthest point from Earth is about 380,000 km.

On November 8, as it nears the moon, the spacecraft’s engine will be fired again to slow the spacecraft, allowing the moon’s gravity to capture it, and then it will go into an initial elliptical orbit around the moon. A group of engineers from JPL are assisting the engineers from India, acting as experienced back-up for the “first-time-flyers” from India. And everything has gone smoothly thus far.

The spacecraft will make observations from the initial orbit, and then the orbit will be lowered a 100 km circular polar orbit. Following this, the Moon Impact Probe (MIP) will be ejected, impacting the lunar surface. Then the main mission will begin with Chandrayaan-1 exploring the moon from orbit with its array of instruments for two years.

Source: Bharat Chronicle

PAMELA Results Mean Only One Thing: Please Trust the Scientific Process

The PAMELA Spacecraft

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Scientists from the PAMELA (Payload for Antimatter/Matter Exploration and Light-nuclei Astrophysics) orbiting spacecraft have published preliminary results, putting an end to months of speculation about the first direct detection of dark matter. The science team was, in essence, “forced” to publish before they had conclusive results because other scientists “pirated” data from the team. “We wanted to make our final results available to the scientific community once the data analysis was finalised,” PAMELA member Mirko Boezio said in an article in Physicsworld.com. “Given that our preliminary conference data are starting to be used by people, we felt this was a necessary step — not least because it provides a proper reference that correctly acknowledges the whole PAMELA collaboration and is available to the scientific community at large.” This is not the way the PAMELA team wanted to present their results, but really, they had no choice.

In a preprint on arXiv, the team says PAMELA has seen more positrons above a certain energy (10GeV) than can be explained by known physics. This excess seems to match what dark matter particles would produce if they were annihilating each other at the center of the galaxy. This excess, the authors say, “may constitute the first indirect evidence of dark-matter particle annihilations.” But they add that there could yet be other explanations, such as that positrons of this kind of energy can also be generated by nearby pulsars.

The science team will need to gather more data and do more work to be able to distinguish between the positron signature of dark matter annihilation and the positron signature of pulsars.

Two previous papers were published based on photos taken of slides of preliminary data that were shown at a science conference by the PAMELA team. See their papers here and here.

We humans are a curious and impatient lot. But we have to allow scientists to do their job, and do it the best way that science allows. Science done right does not mean secrecy or concealment. It means not speculating and waiting to announce results until proof positive. A similar event happened earlier this year with the Phoenix team and the detection of perchlorates. The Phoenix science team was forced to call a press conference to end all the speculation. Right now, the PAMELA team cannot say conclusively one way or the other whether they’ve made a direct detection of dark matter. Given enough time and more data, they will. Unless someone else steals the show again.

Sources: Physicsworld, arXiv, arXiv blog

Microbial Life on the Moon?

Shackelton Crater (and Earth) as seen by Kaguya. Credit: JAXA

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One astrobiologist claims the deep, dark craters on the Moon might contain traces of early life from meteorites blasted off the Earth by asteroids billions of years ago. Joop Houtkooper, from the University of Giessen in Germany says studying these craters could reveal clues about the origin and evolution of life on Earth or even contain remnants of life from other planets in the Solar System, such as Mars. Houtkooper is also one of the few scientists who insist that the experiments done by the Viking Mars Landers in the 1970’s actually did reveal microbial life in the Martian soil, and earlier this year, Houtkooper predicted microbes could be detected by NASA’s Phoenix lander. So, could this new claim about microbes on the Moon be just the latest in a long series of contentious claims, or is Houtkooper onto something?

Houtkooper said the best place for finding evidence of life is on the moon is within the Shackleton Crater at the Moon’s south pole. Houtkooper presented his ideas at the recent 2008 European Planetary Science Congress in Germany. However, this was before results were released from the Japanese Kaguya lunar orbiter, which peered into Shackleton Crater and found no appreciable evidence of water ice. So, while ice on the moon hasn’t been ruled out completely, right now, the evidence isn’t there.

But Houtkooper said the evidence could come in the form of organic molecules, fossil remains, dead organisms, or even organisms in a dormant state that could be revived, such as bacterial spores. He said it is even possible that microbes could have survived for a short while after impact. Although there is no atmosphere to support life today, a temporary, thin atmosphere could have formed shortly after an impact event, as water and gases from the space rock vaporized, Houtkooper claimed.

The permanently shaded craters would be at almost a constant deep freeze temperature of -248ºC, ideal for freezing water and gases such as nitrogen, carbon dioxide or methane, and preserving traces of life undisturbed by sunlight and solar winds.

Other astrobiologists say the theory is possible, but would be a long shot.

“The microbial system on Earth extends to a depth of several kilometers into the crust, and so rocks blasted off the Earth by asteroid impacts could well have contained microbes,” said astrobiologist Malcolm Walter from the University of New South Wales in Sydney.

“I’d be very conservative about this idea,” said Lewis Dartnell, an astrobiologist at University College London (UCL) in the United Kingdom. “If, say, a comet landed right in the middle of a crater, then it’s possible”.

While Houtkooper agreed the idea is controversial, he maintains that there’s a good chance that remains of life could be found – and the latest mission to the Moon could provide the proof. India’s Chandrayaan-1 space probe launched in October will be specifically looking for ice deposits at the lunar poles.

“The long-existing knowledge about the Moon’s rotation axis implies that there are places in eternal shadow at the Moon’s poles,” Houtkooper said. “That means exceptionally low temperatures at, and some depth below, the surface there.”

Source: Cosmos Magazine

The Cosmic Web – NGC 2070 by Joseph Brimacombe

The Cosmic Web - NGC 2070 by Joseph Brimacombe

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Just one glance at this incredible visage is enough to make you do a double take. This intricate net of nebular mists is known as 30 Doradus, or even more commonly as the “Tarantula”, but no space spider created this web. No, sir. What spun out these gossamer strands of HII silk is one of the largest and most active star forming regions known to our local galaxy group…

When Nicolas Louis de Lacaille first saw it in 1751 through his half-inch spyglass, he knew it was something different. He wrote down that it was nebular in nature, without stars and said; “It resembles the nucleus of a small comet.” Too bad he didn’t realize what he was really looking at, for Lacaille was a huge fan of all things science. What he couldn’t see with his primitive telescope is there really is a cluster of stars at the heart of this web… A very compact cluster stars known as R136a. And in its midst? Twelve stars… twelve very massive and luminous stars almost exclusively of spectral type O3. Even at a distance of 180,000 light years these stars light up this nebula so brightly that if it were as close to Earth as the Orion Nebula, it would cast shadows on the night.

So what else lay hidden in the 1000 light year expanse of the cosmic web? Look beyond what you can see in visible light and think like a spider… Try infra-red. With the eyes of the Spitzer Space Telescope aimed towards NGC 2070, scientists could penetrate the dust clouds throughout the Tarantula to reveal previously hidden sites of star formation. Within the luminescent nebula, holes began to appear. These voids are created by highly energetic winds spewing out from the massive stars in the central star cluster. Like the intricate designs woven by the spider, the structures at the edges of these voids are particularly interesting. Dense pillars of gas and dust, sculpted by the stellar radiation, will be the birthplace of future generations of stars!

But like the spider web… It’s a place of death, too.

In 1987 one of the closest supernova events ever to occur near Earth happened in the outskirts of the Tarantula Nebula. The light from the supernova reached Earth on February 23, 1987 and not.since 1604 had humankind been witness to such an event. Even though we were witnessing something that occurred 168,000 years in the past, those X-ray and radio emission were still just as bright as the day the highly energetic electrons and particles spewed into the interstellar medium upon the explosive death of the progenitor star. Oh, there is skeletons in the web, too. Older and weaker supernovae remnants are scattered about, their signatures as faint as the imprint of a fallen leaf that has long blown away. This “Cosmic Web” is home to many supergiant stars. At any moment, a snapshot of any dense region of supergiant stars will show a mixture of newborn stars and supernovae, the signature of stars who those that have lived fast and died young.

Many thanks to AORAIA member, Joe Brimacombe for allowing me to swipe his wonderful image and tell a story.

Where In The Universe Challenge #28

Here’s your image for this week’s “Where In The Universe” challenge. Take a look and see if you can name where in the Universe this image is from. Give yourself extra points if you can name the spacecraft responsible for the image. The new way we’re doing this challenge is that we’ll provide the image today, but won’t reveal the answer until tomorrow. This gives you a chance to mull over the image and provide your answer/guess in the comment section — if you dare. Check back tomorrow on this same post (reminder: no new post tomorrow — come back to this one) to see how you did!

UPDATE (11/6): The answer has now been posted below. If you haven’t made your guess yet, no peeking before you do!!


I have to say, I am impressed with the knowledge of you UT readers! Great job! Yes, it is Tycho’s Supernova Remnant, taken by the Chandra spacecraft. This is a bubble of hot gaseous supernova debris (green and red) inside a more rapidly moving shell of extremely high-energy electrons (blue). These features were created as the supersonic expansion of the debris into interstellar gas produced two shock waves – one that moves outward and accelerates particles to high energies, and another that moves backward and heats the stellar debris. The Chandra X-ray Observatory, which was launched and deployed by Space Shuttle Columbia on July 23, 1999, took this image in 2005.

Learn more about the image here.

And I’m sorry about the delay in posting the answer.