Cassini Spots the Sombrero Galaxy from Saturn

M104 imaged five years apart from Cassini on April 12, 2015 (left) and from the Subaru Telescope on April 12, 2015 (right). Credits: NASA/JPL/SSI/J. Major and NAOJ.

M104 imaged five years apart – from Cassini on April 12, 2015 (left) and from the Subaru Telescope on April 12, 2015 (right). Credits: NASA/JPL/SSI/J. Major and NAOJ.

We’re all used to seeing fantastic images of Saturn and its family of moons from NASA’s Cassini spacecraft, which has spent the last decade in orbit around the ringed world. But every now and then Cassini aims its cameras outwards, capturing images of the sky beyond Saturn – just like we might look up at the stars from here on Earth. And while it’s not designed to be a deep-space observatory like Hubble or Subaru (or even like a modest backyard telescope, really) Cassini can still resolve many of the same stars we can easily see in the night sky… and, on April 12, 2015, it spotted something much farther away: the Sombrero Galaxy (M104), 29 million light-years distant!

Coincidentally Cassini grabbed its image of M104 exactly five years after it was imaged with Japan’s Subaru Telescope, located atop Mauna Kea.

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Curious Stains on Mars’ Summer Slopes Continue to be Seen

Recurring slope lineae (RSL) stain mountain slopes in Hale Crater. (NASA/JPL/University of Arizona)

Recurring slope lineae (RSL) stain mountain slopes in Hale Crater. (NASA/JPL/University of Arizona)

As the midsummer Sun beats down on the southern mountains of Mars, bringing daytime temperatures soaring up to a balmy 25ºC (77ºF), some of their slopes become darkened with long, rusty stains that may be the result of water seeping out from just below the surface.

The image above, captured by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter on Feb. 20, shows mountain peaks within the 150-km (93-mile) -wide Hale Crater. Made from data acquired in visible and near infrared wavelengths the long stains are very evident, running down steep slopes below the rocky cliffs… but the process that’s responsible for them has yet to be confirmed.

Read the rest of my article on Universe Today.

Water Water Everywhere

Earth isn't the only planet with water – we just need to know where to look.

Earth isn’t the only planet with water – we just need to know where to look.

Everyone knows that Earth is a “water-world,” with oceans covering 71% of its surface and at least as much contained within our planet’s mantle deep below its crust. But there’s also liquid water to be found elsewhere in the Solar System: on Mars, on the dwarf planets Ceres and Pluto, and also on the icy moons of Jupiter, Saturn, and Neptune.

NASA is on the hunt for this water, for the main reason that it’s the key ingredient for the evolution of Earth-type life. Where liquid water exists, if there are organic molecules and energy sources as well then the stage is set for life having evolved independently of Earth. And if we can find that that’s the case somewhere, anywhere else in the Solar System, then that would be a huge – no, make that giant – step toward answering the Big Question: are we alone in the Universe?

Today NASA scientists held a conference about the search for oceans beyond Earth, and how we are currently and plan to find out where and how much is (or even was) out there. An infographic accompanied the press materials released.

“What we’re finding out is that the Solar System really is a soggy place.”

– Dr. Jim Green, NASA’s Planetary Science Director

Check out the full infographic below, along with a video of the conference.

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This Was Rosetta’s View of Earth and the Moon in March 2005

The Moon beyond Earth's limb imaged by ESA's Rosetta spacecraft on March 4, 2005 (ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0)

The Moon beyond Earth’s limb imaged by ESA’s Rosetta spacecraft on March 4, 2005 (ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0)

ESA’s comet-chasing Rosetta mission is best known today for its two historic firsts of entering orbit around a comet and sending a lander onto the surface of said comet, in May and November of 2014 respectively. But Rosetta didn’t just go directly from its March 2, 2004 launch to comet 67P; it had to perform several flyby maneuvers beforehand with planets and asteroids on its way out to meet a comet. And now, ESA has shared many of the images acquired during those close passes during its cruise phase in a series of online albums for the public to easily access.

The image above shows the Moon beyond the hazy line of Earth’s atmosphere, acquired on March 4, 2005 during Rosetta’s first gravity-assist flyby of Earth just over a year after its launch. (Rosetta made three such passes by our planet before gathering enough velocity to make it out to 67P!)

See a list of Rosetta’s flybys below and find out how to access the albums.

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NASA’s Next Era Will Rely on Robots

NASA's Robonaut2 faces off with an astronaut in a space suit (NASA/JSC)

NASA’s Robonaut2 faces off with an astronaut in a space suit (NASA/JSC)

NASA’s Shuttle era may be over but its robotic era is in full swing. With robots having long performed the bulk of our exploration across the Solar System, on the surface of Mars, and now assisting astronauts in low-Earth orbit, we’re now also on the verge of having robots doing work for us on the Moon, on asteroids, and even augmenting natural human capabilities to levels otherwise unattainable – especially in the alien environments found outside of Earth.

“This is probably one of the most exciting times to be working at NASA,” said Terry Fong, director of the Intelligent Robotics Group at Ames Research Center. “Regardless of where NASA goes, robots are going to be there. If humans go back to the Moon, or to an asteroid, or Mars, robots are going with them.”

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A Northern View of Saturn’s Stained Moon Iapetus

Saturn's moon Iapetus, imaged by Cassini on March 31, 2015 (NASA/JPL-Caltech/SSI)

Saturn’s moon Iapetus, imaged by Cassini on March 31, 2015 (NASA/JPL-Caltech/SSI)

Here’s a raw image of Saturn’s moon Iapetus, looking down on its northern hemisphere from Cassini on March 31, 2015. The moon’s signature two-toned coloration is evident as its bright icy surface is partially coated by dark material, thought to have been ejected from distant neighbor Phoebe.

Iapetus is 914 miles (1,471 km) in diameter, or about as wide as Texas and Louisiana combined. It orbits Saturn at a considerable distance of 2,212,889 miles (3,561,300 km), which is nine times farther than the Moon is from us.

Iapetus’ north pole is located just below and to the left of the centrally-peaked crater south of the brightest region in the image above. (The two prominent craters near image center are Roland and Turpin.)

Learn more about Iapetus here, and for a color version of the above image click here.

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