Sign up for free Newsletters

Once a month get new photos and expert tips.

Sign Up

Search Results

Results tagged “pictures” from Breaking Orbit

It's tiny, it's pockmarked, and it's got almost no atmosphere. So it's probably small wonder that we cared so little for poor Mercury that we couldn't be bothered to check out a whole half of the planet until 2008.

mercury-global-color.jpg

—Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Arizona State University/Carnegie Institute of Washington

But when we did send a probe to scope out the scene, boy did we find some doozies!

Last October the MESSENGER probe had its second sweep past the planet as it settles into an eventual orbit. Not to waste the opportunity, scientists programed the craft to collect all kinds of data during the brief flyby.

The latest issue of Science describes a whole slew of neat findings from the October visit, including:


I personally loved the magnetic twisters, which I found cool enough to assign as a news story that was deftly reported by our own Rebecca Carroll.

But that last one is also pretty impressive.

As impact basins go, the newly named Rembrandt is a sizable feature—430 miles (700 kilometers) wide, or big enough to stretch from D.C. to Boston if it was on Earth.

rembrandt-basin-earth.jpg

—Image courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/Smithsonian Institution Copyright: Smithsonian Institution

For something so large, it really surprised the research team to find that the floor of the basin has remained largely unchanged for 3.9 billion years.

"This is the first time we have seen terrain exposed on the floor of an impact basin on Mercury that is preserved from when it formed," the Smithsonian's Thomas Watters said in a statement. "Terrain like this is usually completely buried by volcanic flows."

Being almost bare-bottomed means that researchers can see the patterns of ridges and troughs criss-crossing the basin floor, including evidence of a thrust fault that would rival the San Andreas in California.

"The pattern of tectonic landforms in the Rembrandt basin is truly extraordinary," Watters said. "It is unlike anything we have seen before in other impact basins on Mercury, the Moon or Mars, or in basins formed on the icy moons of the outer planets."

There's always a twinkle in a science writer's eye when real life imitates art.

In 2005 we had a snapshot of gases and dust around a star that seemed to be auditioning for the next Lord of the Rings film.

Then in 2007 there came the news that the universe could be packed with double-sunned planets like Star Wars' Tatooine.

Earlier this year a Mars orbiter sent in high-resolution shots of a body called Phobos, highlighting its massive Stickney Crater and its uncanny resemblance to the Empire's ultimate weapon.

phobos-deathstar.jpg

With apologies to Sir Alec Guinness, this time that is a moon—Phobos is the larger of the two known natural satellites orbiting Mars.

—Image courtesy NASA/JPL-Caltech/University of Arizona

Although it was discovered way back in 1877, Phobos has remained fairly enigmatic.

In the late 1950s, its odd orbit inspired Russian astronomers to suggest that the moon is a hollow shell, and an artificial one at that.

It took almost a decade to silence that offbeat theory, based on better calculations of the moon's orbit combined with new density measurements and eventually images from the Viking mission.

But Phobos still boasts some unusual characteristics, prompting much speculation about what the moon is made of and how it took up residence around Mars.

► Read This Entire Post

Sometimes it's possible to be too close to a problem. For example, how would a citizen of Whoville living on a speck of dust know what another speck of dust several light-years away is supposed to look like?

The situation is much the same on Earth.

earth-mars.jpg

Earth, as seen from Mars in 2004
—Image courtesy NASA/JPL/Cornell/Texas A&M

So far we've found more than 300 examples of specks in the distant universe that we have good reason to believe are planets circling other stars—so-called extrasolar planets, or exoplanets.

Almost all of these specks are too far away and/or too small to see directly. But we know they're there, because we can see the gravitational tugs they make on their host stars, or we see a star dim for a bit as a planet passes between it and us.

With current technology, we can tell that quite a few of the worlds we see outside the solar system look a lot like Jupiter, with relatively similar masses, densities, and compositions, but often much closer to their stars than would be expected.

Not long after we spotted the first "hot Jupiter," we found the first exoplanet that looks like it might be a rocky world like Earth, raising hopes that there's at least one distant orb out there that could be habitable for life as we know it.

The problem is, the only habitable world we know of is Earth, and how do we know what Earth looks like from veeeeeery far away?

—Video courtesy NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

Luckily, a few of the orbiters we've sent out to examine the solar system's other denizens are being asked to shoot a few glances back home and give us a better picture of what we should be looking for when scanning the skies for other Earths.

► Read This Entire Post

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.


news.nationalgeographic.com

Share This

Add to Technorati Favorites
 

Subscribe to This Blog

Get the RSS feed for this blog—and don't miss a single word.

RSS     What is RSS?

Blogroll