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August 2009 Archives

Making Babies in Space

Posted on August 27, 2009 | 0 Comments

Alien cultures might be happy to know that if we humans ever do start colonizing the universe, we may have a few problems going forth and multiplying.

A team of Japanese scientists has found that microgravity significantly lowers the birth rate in mammals, based on their study of mice embryos subjected to space-like conditions in the lab.

In previous studies in rats, scientists had seen that microgravity during space flight lowered sperm counts and even caused the poor rodents' testicles to weigh less. [Rat-testicle weigher sounds like a job for Mike Rowe to me!]

Meanwhile, mouse-embryo cells flown aboard the space shuttle Columbia in 1996 failed to yield any mousey babies.

Reporting in the open-access journal PLoS ONE, Sayaka Wakayama, of the Laboratory for Genomic Reprogramming in Kobe, and colleagues note that the issue warrants further study, but sending actual mice into space and seeing if they breed presents a few challenges.

"If mice were to be taken into space, they would be exposed to strong vibrations and hypergravity during the launch, and then suddenly exposed to the additional stress of µG conditions. In these situations, it is highly unlikely that the mice would copulate during the flight period," the study authors write.

The solution? Mouse in vitro fertilization, or IVF.

Using a device that kinda looks like a robot's rotissomat to simulate microgravity, the scientists fertilized mouse embryos and allowed them to develop in conditions like what they would experience in space.

The eggs were then taken out and transferred to waiting mouse moms. The fertilization part worked as expected, and the mice gave birth to 75 healthy space babies.

journal.pone.0006753.g002.jpg

"All these offspring appeared normal, and randomly selected animals were later proven fertile by natural mating," the authors note.

But that's just a 35 percent birth rate, compared to the 63 percent of successfully born IVF mice that got to develop under normal Earth gravity.

Next steps, the authors say, will be to see how well embryo implantation works in space.

If a colony ever does get built on the moon or Mars, I suppose eventually we'll want to extend such studies to humans, although I'm guessing much more work will be done between now and then on whether we can make babies in space the old-fashioned way.

Any volunteers for this important medical research?

Tracking a Mars Rover

Posted on August 17, 2009 | 0 Comments

rover-traverse-map.jpg

—Image courtesy NASA/JPL/University of Arizona

Those of you who think it's cool to drill into Google Maps and find, for example, your car sitting in your driveway, probably know that it's all about coming to a resolution.

The higher a camera's resolution, the more details you can capture in a single image, and the deeper you can zoom in.

Google gets many of its images from Earth-orbiting probes that have eyes sharp enough to see 19.7 inches (50 centimeters) per pixel.

Such satellites have a counterpart orbiting Mars: the High Resolution Imaging Science Experiment, or HiRISE, camera aboard the Mars Reconnaissance Orbiter.

HiRISE can see in resolutions of 9.8 to 19.7 inches (25 to 50 centimeters) per pixel, enough to take snapshots of features as small as an office desk from about 186 miles (300 kilometers) above the planet's surface.

And like Earthlings scanning web maps for their tricked-out Hondas, Mars mission managers can peer into the more detailed shots of the Martian terrain to pick out their vehicles in action.

Case in point: Last week HiRISE treated us to a glorious new shot of Victoria Crater, which the Mars rover Opportunity had risked life and limb to explore in 2007.

Now peer closely at those scalloped edges, and you can just see where it looks like someone was playing connect the dots up near the crater's left-hand rim.

Those are Opportunity's tacks, preserved in the Martian dust after all this time!

rover-tracks.jpg

—Image courtesy NASA/JPL/University of Arizona

After about a year in the crater, the rover clambered back out and headed south, and NASA's been using its orbiters to follow the rover's path since then.

Using such "traverse maps," like the one featured above, Emily Lakdawalla over at the Planetary Society did some heavy lifting and tracked down the rover itself in the full version of the new crater picture.

She's zoomed in so you can clearly see Opportunity ambling across the red planet's dunes after it had stopped to investigate a Martian meteorite.

opportunity-tracks.jpg

—Image courtesy NASA/JPL/University of Arizona

Now is that freakin' sweet or what?

Saturn's Equinox Arrives

Posted on August 10, 2009 | 0 Comments

After a successful four-year mission studying the ringed planet, the Cassini probe was still orbiting Saturn in near perfect health in June 2008. So NASA dug deep and found the funding to keep Cassini gainfully employed.

The extension, dubbed the Equinox Mission, is primarily focused on changes wrought on Saturn by the onset of equinox, when the sun shines directly on the gas giant's equator, which happens just once every 15 years.

In the past Saturn, its rings, and its moons were all illuminated from the south. But tomorrow the equinox comes, and afterward the sunlight will glide over to Saturn's northern face.

Over the long term, Cassini will be able to watch the planet's seasonal changes—at least until the currently funded mission ends in September 2010.

But the time immediately around the equinox is especially exciting, because changes in the planet's position combined with light coming in at different angles are exposing all sorts of 3-D effects in the normally "two-dimensional" rings.

Last week, for example, Cassini images revealed a new itteh bitteh moon hovering just outside Saturn's B ring.

saturn-new-moon.jpg

—Image courtesy NASA/JPL/Space Science Institute, little white arrow courtesy moi

The small, light-colored object is so close to the dense rings—the scientists guess it's a mere 660 feet (200 meters) above—that it was effectively hidden until now.

The unique interplay of light brought on by the upcoming equinox caused the little moon to cast a long shadow on the rings. In general, Saturn's moons cast shadows on the rings only before and after an equinox, so pictures like this are incredibly rare.

That means it's a treat even when bigger, known moons decorate the rings with their own shadowy dances, since the shadows allow Cassini scientists to create unprecedented images with scientific punch.

Here, the moon Tethys casts its spiky shadow across the A and B rings in a mosaic of 17 pictures taken about 2 minutes, 17 seconds apart.

tethys-rings.jpg

—Image courtesy NASA/JPL/Space Science Institute

The changing degrees of light and dark in the same parts of each shadow can tell scientists just how dense the planet's rings are in certain regions.

Saturn's moons also sometimes interact directly with the rings, as seen in this picture of the moon Prometheus creating dark "steamers" through the thin outer F ring.

prometheus-rings.jpg

—Image courtesy NASA/JPL/Space Science Institute

The 53-mile-wide (86-kilometer-wide) moon dips into the F ring when its orbit takes it farthest from the planet. The moon's gravity then pulls material out of the rings as it moves closer to Saturn. (Watch a movie of Prometheus "bouncing" off the F ring.)

So far we've only seen this phenomenon lit from the south, but it's due to happen again late this fall, after the equinox. Scientists hope light coming in from the north will, pardon the cliché, literally shed new light on the moon's effects on the F ring.

As for the equinox itself, Cassini will likely have its eye trained on Saturn to see the gas giant make its roughly 170,000-mile-wide (273,000-kilometer-wide) rings ... disappear!

As wide as the rings are, they're just 30 feet (9 meters) thick. As the planet turns on its axis during the equinox, the edge of the rings will line up with the light from the sun.

It's like turning a piece of white paper edge-on against a mostly white wall and then shining a light directly at it. For all you can see, the paper will seem to vanish.

rings-disappear.jpg

—Image courtesy NASA/Hubble Heritage

Astronomer Galileo Galilei saw this happen in December 1612 (although through his low-power 'scope, he thought the rings were actually two moons on either side of the planet!).

He was appropriately baffled at the vanishing act, writing in a letter: "I do not know what to say in a case so surprising, so unlooked for and so novel."

Sadly the folks at home won't be able to witness the spectacle this year, as Saturn is also in solar conjunction—basically behind the sun as seen from Earth.

So let's all hope Cassini keeps working overtime and catches the equinox in action!

mars-meteorite.jpg

—Image courtesy NASA/JPL-Caltech/Cornell University

Dubbed "Block Island," the conspicuous space rock is now the largest confirmed meteorite found on the red planet, NASA announced today.

The Mars rover Opportunity snapped the above portrait of Block Island on July 31, as it moved in closer to touch the meteorite.

Opportunity's examinations revealed that the two-foot-wide object is an iron-nickel meteorite, although where it came from exactly is still anybody's guess.

Although Opportunity and its twin, Spirit, have found several candidate rocks during their five-plus years on Mars, Block Island is only the second official Martian meteorite.

The first—known as Heat Shield Rock, but formally named Meridiani Planum—was found in late 2004.

On the flip side, meteorites from Mars are also pretty rare, all things considered.

According to NASA, of the 24,000 or so space rocks that have been found on Earth, just 34 are known to be from Mars, presumably broken off from the red planet when something else smashed into its surface.

About This Blog

The moon
From dwarf planets to hot Jupiters, join NatGeo News space and tech editor Victoria Jaggard in a global discussion about all things extraterrestrial.


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