Moons Large and Small

[/caption]

It may be one of the best images from Cassini yet this year! Cloud-covered Titan and tiny Prometheus (can you see it just above the rings on the right?) are literally dwarfed by their parent Saturn in an image captured on Jan. 5, 2012.

Prometheus’ pinpoint shadow can also be seen on Saturn’s cloud tops, just inside the thin, outermost F ring shadow at bottom left.

The two moons themselves couldn’t be more different; Titan, 3,200 miles (5,150 km) wide, is wrapped in a nitrogen and methane atmosphere ten times thicker than Earth’s and is covered with vast plains of dark hydrocarbon dunes and crisscrossed by rivers of liquid methane.

Prometheus imaged by Cassini in Dec. 2009.

Prometheus, on the other hand, is a potato-shaped shepherd moon 92 miles long and 53 miles wide (148 x 53 km) that orbits Saturn just inside the narrow, ropy F ring. While it doesn’t have an atmosphere, it does create some impressive effects on the icy material in the ring!

Another moon, Pandora, casts its shadow onto Saturn just outside the F ring shadow at bottom center. 50 miles (80 km) wide, Pandora shepherds the outer edge of the F ring but is itself not visible in this image. Watch an animation here.

This image was featured on the Cassini Imaging Central Laboratory for Operations (CICLOPS) website on Feb. 28, 2012. The view looks toward the southern, unilluminated side of the rings from about 1 degree below the ringplane.

Image credit: NASA / JPL / Space Science Institute.

Heads Up: It’s Another Mind-Blowing Aurora Photo

"Forest Storm" by Ole Salomonsen (arcticlightphoto.no)

[/caption]

Photographer Ole Christian Salomonsen is a master at capturing the northern lights in all their glory… as this image once again shows.

Ole describes the story behind this photo:

“Shot at the end of a ‘weak’ aurora night in Muonio, Finland. Took this at outside the cabin I was staying at close to Harriniva. The outburst came from an CME that first started disappointingly weak. I was about to go to bed but thought I should wait just a little more and see. Man am I glad I waited!!”

Man, are we glad too! Thanks for sharing these amazing views with us Ole, and keep up the great (and chilly) work!

Image © Ole Salomonsen. Used with permission. See more of Ole’s work on www.arcticlightphoto.no.

Salty Soil on Mars Could Be Slurping Water from the Atmosphere

This image provided by NASA shows a scraped area on Mars known as "Snow White," photographed on July 8. Two samples from Snow White were delivered to the Phoenix Mars Lander's wet-chemistry lab, and tests turned up evidence of perchlorate. Credit: NASA/JPL/University of Arizona

[/caption]

It happens every summer in humid air: the salt in your salt shaker clumps together as the salt draws in the water from the air. Researchers have found this happens even in the frigid but dry McMurdo Dry Valley in Antarctica, a cold, polar desert. The sandy, salty soils there are frequently dotted with moist patches in the spring despite a lack of snowmelt and no possibility of rain. What was discovered is that the salty soils in the region actually suck moisture out of the atmosphere. Salty soils were found on Mars’ polar region by the Phoenix lander, so could the same thing be happening on the Red Planet, creating a salt brine within Mars’ soil? And if so what are the implications for life forming there?

Joseph Levy, a post-doctoral researcher from Oregon State University said it takes a combination of the right kinds of salts and sufficient humidity to make the process work. But those ingredients are present on Mars.

“If you have sodium chloride, or table salt, you may need a day with 75 percent humidity to make it work,” he added. “But if you have calcium chloride, even on a frigid day, you only need a humidity level above 35 percent to trigger the response.”

The soils in Antarctica have salt from sea spray and from ancient fjords that flooded the region. With enough humidity, those salty soils suck the water right out of the air, forming a brine, Levy said, that will keep collecting water vapor until it equalizes with the atmosphere.

Levy and his colleagues, from Portland State University and Ohio State University, found that the wet soils created by this phenomenon were 3-5 times more water-rich than surrounding soils – and they were also full of organic matter, including microbes, which they said could enhance the potential for life on Mars. The elevated salt content also depresses the freezing temperature of the groundwater, which continues to draw moisture out of the air when other wet areas in the valleys begin to freeze in the winter.

Though Mars, in general, has lower humidity than most places on Earth, studies have shown that it is sufficient to reach the thresholds that Levy and his colleagues have documented in Antarctica.

The parallels of what was found by the Mars Phoenix team is striking. The salty perchlorates found on Mars by the Phoenix lander also strongly attracts water and makes up a few tenths of a percent of the composition in all three soil samples analyzed by Phoenix’s wet chemistry laboratory. Principal investigator of the Phoenix mission, Peter Smith from the University of Arizona, Tucson, said the perchlorates could pull humidity from the Martian air.

A paper about Phoenix water studies, led by Smith, cites clues supporting an interpretation that the soil has had films of liquid water in the recent past. The evidence for water and potential nutrients “implies that this region could have previously met the criteria for habitability” during portions of continuing climate cycles.

At higher concentrations, it might combine with water as a brine that stays liquid at Martian surface temperatures. Some microbes on Earth use perchlorate as food, and future human explorers on Mars might find it useful as rocket fuel or for generating oxygen.

Levy and his team discovered the mysterious patches of wet soil in Antarctica, and then explored the causes. Through soil excavations and other studies, they eliminated the possibility of groundwater, snow melt, and glacial runoff. Then they began investigating the salty properties of the soil, and discovered that the McMurdo Dry Valleys weather stations had reported several days of high humidity earlier in the spring, leading them to their discovery of the vapor transfer.

“It seems kind of odd, but it really works,” Levy said. “Before one of our trips, I put a bowl of the dried, salty soil and a jar of water into a sealed Tupperware container and left it on my shelf. When I came back, the water had transferred from the jar to the salt and created brine.

“I knew it would work,” he added with a laugh, “but somehow it still surprised me that it did.”

The salty soils also are present on the Red Planet, which makes the upcoming landing of the Mars Science Laboratory this summer even more tantalizing.
Evidence of the salty nature of the McMurdo Dry Valleys is everywhere, Levy said. Salts are found in the soils, along seasonal streams, and even under glaciers. Don Juan Pond, the saltiest body of water on Earth, is found in Wright Valley, the valley adjacent to the wet patch study area.

“The conditions for creating this new water source into the permafrost are perfect,” Levy said, “but this isn’t the only place where this could or does happen. It takes an arid region to create the salty soils, and enough humidity to make the transference work, but the rest of it is just physics and chemistry.”

The study by Levy and his team was published online this week in the journal Geophysical Research Letters.

Sources: University of Oregon, previous article about the Phoenix Lander

Our Early Universe: Inflation, or Something Totally Wacky?

A schematic look at the universe - where it came from and where it is now. Credit: NASA.

[/caption]

Astronomers generally accept the theory that our universe looks the way it does because of cosmic inflation — rapid expansion in the moments after its birth. This explains the expanse and apparent flat shape of the universe observed through instruments like NASA’s Wilkinson Microwave Anisotropy Probe. But inflation isn’t the only model that explains the early universe. There are others, and they get wacky. 

Three physicists from the University at Buffalo — Ghazal Geshnizjani, Will Kinney and Azadeh Moradinezhad Dizgah — set out to investigate other cosmic models. Their study titled “General Conditions for Scale-Invariant Perturbations in an Expanding Universe” appeared in November in the online Journal of Cosmology and Astroparticle Physics (not to be confused with the Journal of Cosmology) and contained some interesting results.

This picture of the infant universe from NASA's Wilkinson Microwave Anisotropy Probe (WMAP) reveals 13 billion+ year old temperature fluctuations that correspond to the seeds that grew to become the galaxies. Credit: NASA Goddard Space Flight Center.

They stuck with the basics — that the theory of gravity is correct and that the early universe did rapidly expand. With these two constraints, the team found that only three models explain the early universe and the distribution of matter we observe today. But these models require very strange physics.

According to their calculations, the early universe required an accelerated cosmic expansion (inflation), a speed of sound faster than the speed of light, or extremely high cosmic energy to end up with our current universe. The third model actually demands such high energy that scientists would need to invoke a theory of quantum gravity like string theory to explain the extra dimensions of space-time that would pop up.

The takeaway message? Inflation turns out to be the only way to explain the universe within the context of standard physics, said Kinney. He allows that someone might come up with exotic physics to explain or create other models, like a speed of sound faster than that of light, but suspects people are more comfortable working with models that fit within commonly accepted laws of particle physics.

The difficulty of explaining other models, said Kinney, “puts the idea of inflation on a much stronger footing, because the available alternatives have problems, or weirdnesses, with them.”

Cosmic inflation incorporates quantum field theory to explain the distribution of matter in the universe. Under normal circumstances, particles of matter and antimatter can pop into existence suddenly before colliding and annihilating each other instantly. These pairs flew apart so rapidly after the universe’s birth that they didn’t have a chance to recombine. The same theory applies to gravitons and antigravitons, which form gravity waves.

These particles of matter are the basis of all structure in the universe today. Tiny fluctuations cause matter to collapse and form stars, planets, and galaxies.

But the hunt for other viable models continues. Kinney for one isn’t finished exploring other theories, including those that rely on superluminal sound speeds. There may yet be some major changes to our understanding of the cosmos.

Source: The University of Buffalo

Today’s Martian Weather: Partly Cloudy

Clouds obscure the surface of Mars (NASA/JPL/ASU)

[/caption]

Changing seasons in Mars’ northern hemisphere brings a change in the weather, and the clouds have rolled in to cover part of the polar surface in this intriguing image from the Mars Odyssey spacecraft.

Mars Odyssey’s THEMIS visual imager (VIS) captured this image on Jan. 24, 2012, as it passed over the Red Planet’s northern pole during one of its 2-hour-long orbits.

Clouds on Mars have been seen before, both from orbit and from the surface. They are made up of fine water ice particles and are usually at altitudes of 10 to 15 km high. Read more about Martian weather here.

The full THEMIS scan of the area is below.

Martian polar clouds as seen by THEMIS

The area imaged is about 21 km wide by 73 km high  (13 x 45 miles).

Image credit: NASA / JPL / Arizona State University. Hat-tip to Mr. Bill Dunford at Riding With Robots (@ridingrobots). 

Just In From SpaceX: Dragon and Falcon 9 Assembly Now Complete

Dragon spaceship and Falcon 9 rocket just completed assembly at Cape Canaveral on Feb. 27, 2012. Credit: SpaceX, via @SpaceX

[/caption]

Today SpaceX today released an image of the fully assembled Dragon capsule and Falcon 9 rocket inside their facility at Cape Canaveral. This means the first test launch of a commercially built spacecraft to the International Space Station is just a bit closer. The exact date of the launch has not yet been announced after NASA and SpaceX agreed in early this year that the Feb. 7 date they were aiming for was not feasible. The demonstration flight – called COTS 2/3 – will be the premiere test flight in NASA’s new strategy to resupply the ISS with privately developed rockets and cargo carriers under the Commercial Orbital Transportation Services (COTS) initiative.

In a press conference earlier this month, NASA’s Mike Suffredini said SpaceX’s launch would be no earlier than March 20. “There are no big problems being worked but a lot of little things to wrap up,” he said. “I wouldn’t hold my breath, as it is a challenging date, but I would guess we’ll fly within a couple of weeks of that date. We’ll hold that date as we work towards the launch.”

Suffredini added that SpaceX is working on minor hardware modifications, plus they will need to do a wet dress rehearsal and hot fire test beforehand, so all that makes March 20 a challenging date. There’s a good window of opportunity between March 20 and the next Soyuz launch to bring the next crew to the ISS, which has been delayed due to problems with the Soyuz capsule. No firm date has been set for the Soyuz launch, but it will likely be late April or early May.

We’ll keep you posted when the tentative launch dates are announced.

And if you haven’t seen it yet, click on the image below to see a very cool panorama of the inside of the Dragon capsule.

Click to see an interactive panorama for a look inside Dragon in its cargo configuration, as it will be on its first mission to the International Space Station:

Source: @SpaceX

Carnival of Space #238

Carnival of Space. Image by Jason Major.

[/caption]

This week’s Carnival of Space is hosted by Brian Wang at Next Big Future.

Click here to read the Carnival of Space #238.

And if you’re interested in looking back, here’s an archive to all the past Carnivals of Space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, sign up to be a host. Send and email to the above address.

The Best ISS Video Ever? You Decide.


Is this the best video footage ever of photos taken from the International Space Station? ISS astronaut and Expedition 29 commander Mike Fossum seems to think so.

If anyone would know what a good ISS video is, he would! So watch, and decide for yourself.

Video uploaded by YouTube user bitmeizer. Made from sequences of still photographs taken by Expedition 29 crew members, the time-lapse videos have been digitally smoothed out and a soundtrack added, along with some transition effects.

Original video segments courtesy of the Image Science & Analysis Laboratory, NASA Johnson Space Center. See more at the Gateway to Astronaut Photography of Earth.

Face-to-Face With Some Shattered Lunar Boulders

The remains of crumbled boulders in Schiller crater (NASA/GSFC/Arizona State University)

[/caption]

Breaking up may be hard to do, but these two lunar boulders seem to have succeeded extremely well! Imaged by the Lunar Reconnaissance Orbiter Camera (LROC) in October of 2009, this crumbled couple was recently identified by Moon Zoo team member Dr. Anthony Cook and brought to the attention of the project’s forum moderator.

The tracks left in the regolith — lunar soil — behind the boulders tell of their past rolling journeys down the slope of the elongated Schiller crater, in which they reside. Rolling boulders have been spotted before on the Moon, but what made these two split apart? And…why does that one on the lower right look so much like half a face?

Several things can cause lunar boulders to come loose and take the nearest downhill course. Meteorite impacts can shake the ground locally, giving the rocks enough of a nudge to set them on a roll. And moonquakes — the lunar version of earthquakes, as the name implies (although not due to tectonic plate shifts but rather to more mysterious internal lunar forces) — can also dislodge large boulders.

The low gravity on the Moon can make large rocks take a bounding path, evidenced by the dotted-line appearance of some of the trails.

Could all that bounding and bouncing have made the two boulders above shatter apart? Or was something else the cause of their crumbling?

Dr. Cook suggested that the boulders could have fractured before they began rolling, and then the added stress of their trip down the crater’s slope (uphill is to the right) made them break apart at the end of their trip… possibly due to further weathering and the extreme temperature variations of lunar days and nights.

Although a sound idea, Dr. Cook added, “I’m a bit puzzled though why the one on the top left has rock debris so far away from the centre. The boulder that looks like a skull rock on the bottom right has debris a lot closer to it, that could simply be explained by bits falling off as one would expect from the explanation above.”

This is one rock that's not happy about its breakup!

Another idea is that the boulders were struck by meteorites, but it seems extremely improbable that two would have been hit right next to each other. Still, not impossible, especially given the geologic time spans in play.

And as far as the “skull rock” boulder is concerned… that’s a little something called pareidolia, the tendency for our brains to interpret random shapes as something particularly significant. In this case it’s a human face, one of the most popular forms of pareidolia (perhaps best known by the famous “Face on Mars”, which, as we all now know, has been since shown to be just another Martian mesa.)

It does look like a face though, and not a particularly happy one!

Find out more about rolling boulders and Schiller crater on the LROC site hosted by Arizona State University here, and take a look at the full image scan of the region yourself… you may find more of these broken-up rolling rocks!

LROC WAC global 100-meter mosaic image of the 180-km long, 70-km wide Schiller crater. Overlaid onto a laser altimetry elevation model. (NASA/GSFC/Arizona State University)