More Amazing Images of Iapetus

2007-0913iapetus.thumbnail.jpg

We asked, and Cassini delivered; amazing, intriguing images of the surface of Saturn’s moon Iapetus. The spacecraft completed its latest flyby on September 10th, 2007, skimming just 1,640 km above the moon’s surface. Scientists will be digesting the photographs for years.

During this most recently flyby, Cassini passed 100 times closer than its previous Iapetus flyby in 2004. At this distance, the spacecraft was able to reveal the moon’s strange bulging shape, equatorial ridge, and pattern of bright and darkness across its features.

Many of its photographs focus in on the bizarre mountain ridge that circles the moon’s equator, like a seam. The new Cassini images showed that this ridge is mountainous, rising as high as 20 km, and extends across more than half its circumference.

Mountains on Iapetus. Image credit: NASA/JPL/SSI
The mystery deepens with the unusual light and dark hemispheres of Iapetus. One side is as white as snow, and the other is as black as tar. With the new Cassini images, you can actually see where the different regions mix. On the dark side, you can see spots where there are patches of white ice on dark mountainsides. And then on the bright side, you can see blobs of dark material. This dark material forms a very thin coating; probably only a few metres deep, since there are regions where impact craters have punched right through it, revealing white material underneath.

What caused this material? That’s a mystery. Maybe some previous Saturnian moon broke up, and spray painted Iapetus. Or maybe the material is volcanic material that welled up from within the moon. And this could somehow be connected with the moon’s equatorial ridge.

The images from Cassini were actually delayed early Tuesday, because a cosmic ray hit the spacecraft, putting it into safe mode. This happened after it had captured all its images from its flyby, and they were safely stored in memory. After a few hours Cassini came out of safe mode and continued sending its data back to Earth.

Original Source: ESA News Release

Planet Survives its Star Becoming a Red Giant

2007-0913planet.thumbnail.jpg

When a star like our own Sun nears the end of its 10 billion year life, it expands up into a red giant, consuming any planets foolish enough to orbit closely. But what happens to the more distant planets? Astronomers have discovered just such a planet, orbiting a red giant star. Perhaps this gives us hope for the fate of our own planet Earth, when the Sun expands too. Not so fast.

An international team of astronomers from 15 different countries announced the planetary discovery, and their article will be published in the September 13th edition of the journal Nature.

The planet is called V 391 Pegasi b, and before its parent star transformed into the red giant we see today, it orbited at roughly the same distance as the Earth. As the star expanded, its centre of gravity changed, and the planet’s orbit spiraled outward, keeping pace with the changing star. Although the star now engulfs a distance comparable between the Sun and the Earth, the planet is now out past the orbit of Mars; takes 3.2 years to complete a full year.

So does this mean the Earth’s safe? Not so fast. Here’s one of the researchers, Steve Kawaler from Iowa State University:

“We shouldn’t take too much heart in this – this planet is larger than Jupiter, so a smaller planet like the Earth could still be vulnerable. As far as our planets are concerned, we expect Mercury and Venus to disappear in the Sun’s envelope, whereas Mars should survive. The fate of the Earth is less clear because its position is really at the limit: it appears more likely that the Earth will not survive the red giant expansion of the sun either, but it is not for sure.”

Finding this planet was incredibly laborious work. It took seven years of observations and calculations to confirm its existence. It also marks the first time that a new technique was used to discover planets. Traditionally, astronomers measure the change in a planet’s velocity as it’s yanked back and forth by the gravity of a large planet using a technique called spectroscopy, where the spectrum of its light shifts. In the case of V391 Pegasus b, the astronomers measured small variations in timing of light coming from the star to determine its velocity.

Original Source: University of Delaware News Release

Google Pledges $30 Million for Private Moon Rover Prize

2007-0913google.thumbnail.jpg

Are you working on anything right now? If you’ve got a little time to kill between now and 2012, you might want to win the newly announced $30 million prize announced by the X-Prize Foundation and Google. You’ll need some engineering expertise as well; in order to take the prize home, you’ve got to land a rover on the Moon, capture some video, and drive around a little – maybe find some water ice while you’re at it.

The newly announced Google Lunar X Prize isn’t a single $30 million prize. In fact, it’s actually a collection of prizes. The main prize is $20 million, awarded to the first team that can soft land a privately funded spacecraft onto the surface of the Moon, and then drive a rover 500 metres transmitting video and images back to Earth. If nobody claims the prize by 2012, it will shrink to $15M and go until the end of 2014.

Unlike the Ansari X-Prize, which offered $10M to the first privately built craft to reach 100 km altitude, the Google Lunar X-Prize does award a second place finisher. The second team to put a rover on the surface of the Moon will take home $5M.

They’ve also announced a series of bonus prizes totaling $5M for other completed tasks, such as surviving the lunar night (14.5 days), driving further on the Moon, capturing images of Apollo hardware, and discovering deposits of water ice.

Needless to say, the skills and resources required to accomplish a goal like this are massive. Traditionally it requires the resources of government and the entire populations of countries. If a private firm could accomplish this on a reasonable budget, it would be a tremendous accomplishment for private space exploration.

Original Source: Google Lunar X-Prize News Release

Dawn is on the Launch Pad

2007-913.thumbnail.jpg

Despite delays and near cancellation, NASA’s Dawn spacecraft is now on the launch pad, all ready to begin its mission to two of the largest asteroids in the Solar System. If all goes well, Dawn will blast off as early as September 26th from Cape Canaveral aboard a Boeing Delta II rocket. Next stop, Asteroid Vesta.

The Dawn spacecraft, fixed atop its Boeing Delta II launcher made the 25-km journey from Astrotech Space Operations to Pad-17B at Cape Canaveral on Tuesday. Before it launches on September 26th, engineers will perform a final test to simulate the launch – without rocket fuel, of course.

The September 26th launch window opens up at 7:25 am EDT, and stays open for 29 minutes. A similar window is available on following days until its launch period closes entirely on October 15th. It’s got to launch between those dates to have the right trajectory to complete its mission.

Dawn’s mission is to journey to, and orbit two separate asteroids in the Solar System: Ceres and Vesta. No other spacecraft has ever orbited two bodies after it’s left the Earth. Although they’re both asteroids, the two formed under different conditions in the early Solar System. So this single spacecraft will get able to orbit each in turn and study their chemical makeup and take detailed images of their surface.

Original Source: NASA/JPL News Release

Pulsar Has Almost Completely Devoured a Star

2007-0912pulsar.thumbnail.jpg

Astronomers using NASA’s Swift and Rossi X-ray Timing Explorer satellites have discovered a very bizarre object. It only has about 7 times the mass of Jupiter, but instead of orbiting a star, it’s orbiting a pulsar. Oh, and it’s not a planet. It’s all that’s left from a star after the pulsar siphoned away most of its material.

The ghastly duo was discovered on June 7 when Swift picked up a burst of X-rays and gamma rays coming from the direction of the galactic centre. Rossi turned to gaze at the source as well, and confirmed that it’s pulsing out X-rays 182.07 times a second. These are the classic characteristics of a pulsar – the rapidly spinning remains of a massive star.

Normally a pulsar like this is slowing down over time, releasing energy that decreases its rotational velocity. However, in the case of SWIFT J1756.9-2508, it’s actually speeding up. This means that some source is supplying the pulsar with additional material to increase its spin rate.

The researchers were able to detect that a low mass object is orbiting the pulsar, tugging it back and forth, towards and away from the Earth. Astronomers were then able to calculate that this binary companion has somewhere between 7 and 30 times the mass of Jupiter.

The system probably formed billions of years ago as a very massive star and a smaller companion with 1 to 3 solar masses. The massive star evolved quickly and then detonated as a supernova. The smaller star eventually died as well, becoming a red giant, and encompassing the pulsar. This slowed down their orbits enough to begin them spiraling inward.

Today they’re so close that the pulsar produces a tidal bulge on the surface of the dead star, siphoning material away. Sometimes there’s so much mass accumulated that it piles up and explodes as the outburst that led astronomers to the discovery in the first place.

Don’t think of the companion as a planet. “Despite its extremely low mass, the companion isn’t considered a planet because of its formation,” says researcher Christopher Deloye of Northwestern University. “It’s essentially a white dwarf that has been whittled down to a planetary mass.”

Original Source: NASA News Release

Mars Has Had Many, Many Ice Ages

2007-0912marsice.thumbnail.jpg

The polar ice caps on Mars have been there for a long time; although, they haven’t always stayed the same size, or shape. They cover the surface between the poles and approximately 60° latitude today, but Norbert Schorghofer of the Institute for Astronomy and NASA Astrobiology Institute in Hawaii has shown that Mars has had at least forty major ice ages during the past five million years.

The Martian ice caps are divided into three layers: a massive bottom sheet, a porous middle layer and a thin, dry, dusty top layer. The makeup and extent of the ice coverage has varied over its long history due to both precipitation of water vapor from the atmosphere, and the diffusion and condensation of water from pores in the ice.

“Although neither of the two mechanisms by itself could simultaneously account for the mass fraction and latitudinal boundary of the observed ice, their combination provides just enough ice at the right places,” Schorghofer said.

Unlike the Earth, Mars doesn’t have a Moon to keep its tilt in check. Instead, the planet is able to tilt as much as 10-degrees from its current angle. This can create tremendous variation in the size of its ice sheets.

Earlier studies of the ice showed that the shifting of the ice was due largely to Mars’ varying tilt (obliquity), and thus changes in global and local temperatures affecting the humidity levels of the entire planet. Schorghofer used computer modeling that takes into account thermal and atmospheric conditions, as well as the growth and retreat of the ice sheets. His research shows that the transfer of water vapor from the ice into the atmosphere, and the condensation of this water back into the ice profoundly altered the way in which the ice caps melted and re-froze.

Closer to the poles, the amount of ice changes very little over time. But near the edges of the sheets, the volume of ice has varied by as much as 100,000 cubic km during each ice age. Mars’ icy love handles have each also shrunk an overall depth of 60cm over the past 2.5 million years.

Understanding the cause for ice ages on Mars may help us learn more about the climate history of other planets, including Earth.

“The dynamic nature of the ice sheets makes Mars an ideal system in which to test and expand our knowledge of astronomical climate forcing. A great deal could be learned about terrestrial ice ages from the study of Martian ice stratigraphy – a longer, cleaner and simpler record than Earth’s,” Schorghofer said.

When the Phoenix Mars Lander arrives at the Red Planet in 2008, it might just see the different kinds of ice layers that Schorghofer is predicting.

Original Source: IfA

Opportunity is Entering Victoria Crater

2007-0912rover.thumbnail.jpg

With the powerful Martian dust storms dissipating, the Mars Exploration Rovers are ready to resume their duties, apparently no worse for wear. When we last met our heroes, Opportunity was about to climb down into Victoria Crater to look for evidence of ancient water. Now it took its first tentative steps into the crater, putting all six wheels onto the slope. And then it crawled back out again. Easy does it…

Victoria Crater measures 800 metres (half a mile) across, and it’s the largest impact crater either of the rovers have encountered during their travels on Mars. Since the crater cuts down through Martian rock, it gives scientists an unprecedented opportunity to peer back in time, when layers of rock were put down – ideally when there was liquid water present.

The rover team commanded Opportunity to drive just far enough on September 11, 2007 that all six of its wheels got onto the inner slope. The rover was then asked to come back out again, so the team could measure the amount that its wheels slipped on the slope. Right at the end, as Opportunity was just crawling out, its wheels slipped further than the rover team wanted, so they had it stop, with its front wheels still on the slope.

Now that they’ve gathered data on Opportunity’s traction on this angle, the rover team will analyze it to understand if entering or exiting the crater is going to pose a hazard.

Original Source: Rover status report

Hubble Looks at Four Dead Stars

2007-0911hubble.thumbnail.jpg

Planetary nebulae are some of the most beautiful objects in the Universe. Don’t let the name confuse you, though, they have nothing to do with planets. They’re all that’s left behind when stars at the end of their lives cast off their outer layers into space. Here’s a nice image released from the Hubble Space Telescope, containing 4 different planetary nebulae.

As a star like our Sun reaches the end of its long life, its ejects its outer layers in a series of dramatic events. The ultraviolet light from the star illuminates the material, causing it to glow like we see in this Hubble photograph. This same ultraviolet light also disperses the cloud of material, pushing it outward so that it eventually fades away into the vacuum of space.

Although the star might have lived for 10 billion years, its planetary nebula lasts for just a moment – only 10,000 years.

In this Hubble image there are 4 planetary nebula.

At the top left is He 2-47, nicknamed the “starfish” because of its shape. It has six different lobes, which indicates that the original star shed material three different times in three different directions. With each ejection event, the star blasted out twin jets of material.

At the top right is NGC 5315, which seems to have an x-shaped structure. As with the previous nebula, it suffered two different ejection events, casting away its outer layers and firing out jets in opposite directions.

IC 4593 is on the bottom left, and it’s in the northern constellation Hercules. My good friend Phil Plait actually did a cool write up about this object, so I link you to his site for the scoop.

And finally, NGC 5307 is down at the bottom right, and has a beautiful spiral pattern. The dying star might have had a serious wobble as it was expelling gas, creating the complex shapes in the picture.

Original Source: Hubble News Release

Meteoroids Carve Tunnels as They Burrow Through the Atmosphere

2007-0911meteor.thumbnail.jpg

Every day, material is raining down on the Earth. Fortunately, we’ve got an atmosphere to protect us. As the tiny particles impact the atmosphere, air piles up in front of them, heating up, and blazing a trail in the sky. That’s a meteor. According to a team of Japanese researchers, as the micrometeoroids rain down, they carve out tiny tunnels just a few millimetres across.

Astronomers used to believe that meteors opened up gaps in the atmosphere less than a metre across, but they weren’t exactly sure how wide they really were. But new observations from the powerful Subaru telescope located atop Mauna Kea, Hawaii have narrowed the size down to just a few millimetres.

Observing meteors with the Subaru telescope is actually very difficult. It was designed to observe deep space astronomical objects, nothing as close as the Earth’s atmosphere. This means that the meteor trails look blurry. Even observations of satellites look blurry. Despite the blur, the researchers were able to get their data.

Over the course of a 19-hour observation, 13 meteor tracks were observed. Scientists then carefully analyzed the images, to see how many photons were released as the meteor passed through the atmosphere. Based on the number of photons they detected, the researchers were able to calculate that the trails are just a few millimetres across.

Original Source: Subaru News Release

The Triangle that Skimmed Past the Earth: Asteroid 2002 NY40

2007-0911asteroid.thumbnail.jpg

In August 2002, a bizarre looking asteroid made its closest approach to the Earth, skimming only 540,000 km above the Earth’s surface. That’s only 1.5 times the distance between the Earth and Moon. This gave astronomers an unprecedented opportunity to study the asteroid as it zipped past. Perhaps its most unusual feature? It’s shaped like a triangle.

Asteroid 2002 NY40 was first discovered as part of the automated LINEAR system in New Mexico on July 14, 2002. And then, just a month later it made this closest approach, coming within 540,000 km of the Earth. As it approached, it gained in brightness, reaching as high as 8th magnitude – not visible with the unaided eye, but easy to spot with binoculars or a backyard telescope (if you knew where to look).

2002 NY40’s close approach was a rare event. Near Earth asteroids only get this close once every 50 years or so. The last asteroid to get this near was NEA 2001 CU11 which passed just outside the Moon’s orbit on August 31, 1925. And it wasn’t discovered for 77 years after it made the flyby – astronomers had to go back and calculate when it passed us by.

On the evening of August 17/18, 2002 NY40 was scheduled to make its closest approach. During this night, astronomers around the world, including a team of researchers from Boeing and the US Air Force focused in on it. The Boeing/Air Force team brought the 3.6 metre AEOS Adaptive Optics telescope in Hawaii to bear and studied the asteroid in unprecedented detail, revealing a tremendous amount of surface features. With all this data, they were able to better understand the physical makeup of the asteroid, and get an idea of its structure. Their results will be published in an upcoming issue of the journal Icarus.

Oh yeah, and it looks like a triangle.

The first observations were made with the Raven telescope located at the Remote Maui Experiment site at the base of Haleakala in Kihei, Hawaii. The telescope was configured so that it could track a fast moving object, like 2002 NY40 as it moved quickly through the telescope’s field of view. The researchers modified their exposure times dynamically – ranging from 15 seconds to 60 seconds – as the asteroid came and went. This allowed them to get the same amount of light for every image; it let them compare apples to apples.

Getting these high resolution images of the asteroid was actually pretty difficult. At its very brightest, closest point, when Asteroid 2002 NY40 could be seen at the greatest resolution, it was moving very quickly across the sky – it covered the diameter of the Moon every 6 minutes, zipping across the sky at 65,000 km/hour. The background stars changed with every image. Instead of calibrating against a single set of background stars, the researchers had to calibrate each image against whatever images happened to be in the field of view at the time.

Asteroid 2002 NY40 is tumbling. Its main rotation takes about 20 hours, and its secondary rotation takes about 18.5 hours. Living on this asteroid would be disorienting, to say the least.

According to the best images, 2002 NY40 is about 800 metres across. Once again, this was challenging to discern because the asteroid was casting shadows on itself for part of the flyby. Only at the moment of its closest approach, were astronomers able to get a good image showing its size. This team’s estimates are actually much larger than previous estimates, which calculated it being 250-450 metres.

It turns out, astronomers were quite lucky with the flyby. 2002 NY40 was perfectly positioned during its closest approach to present its largest face to the Earth. With this much data, the researchers were able to classify it as a Q-type asteroid; an uncommon class of inner-belt asteroids that have some metal in them.

And of course, one of the most amazing observations is its strange triangular shape. Getting these images out of the raw data was the hardest part. Lewis Roberts, one of the researches that did the work remarked that, “the imaging was the most challenging. It was a difficult object to acquire good data on and the raw data did not look great. The image processing was top notch and pulled out some good images.”

Original Source: Arxiv Paper