The image above shows what New Horizons looks like to the new Allen Telescope Array which has just come online this fall. The array is currently a collection of 42 antennas which will grow to around 350 over time and it will begin to scan the sky for signs of intelligent life like the one shown above. According to Seth Shostak of SETI, if you draw out some well respected formulas to their logical conclusions… you should be looking at mankind discovering evidence of intelligent life somewhere inside of 20 years from now.

See the full article at Universe Today.

On the Phoenix Mission’s 152nd Sol (a Martian day) the lander has fallen silent and mission engineers have been unable to communicate with it for over a week. This was expected as the Martian sunlight is less and less as the season changes. The sun is simply not providing enough energy to replenish its solar batteries. There is an outside chance that communications might resume again, but it would be a fleeting opportunity at best.

In all, the mission prooved the existence of water-ice in the Martian subsurface; we saw (with our own eyes) Martian ice melting; it was the first time an atomic force microscope was used outside the bonds of Earth; the discovery that Martian soil may not be that different from the Earth’s and that growing plants in it may not be at all difficult; Phoenix found trace amounts of salt which could be nutrients for life; and finally calcium carbonate which suggests a past existence of liquid water on the surface of an anchient Mars.

And who could forget this image. Not too shabby.

Tomorrow’s Cassini buzz of Enceladus is closer than ever not only at Enceladus, but at any other body in the Saturnian system. It is to come only 25km from the surface. It is to fly deep into the plumes, but this visit is more about smell than vision. Imagery is not expected to be as impressive as August’s pass despite the close proximity due to the spacecraft‘s instruments concentrating on particles and dust analysis and not pretty pictures.

“most of the terrain east of Kuiper, toward the limb (edge) of the planet, the departing images are the first spacecraft views of that portion of Mercury’s surface. A striking characteristic of this newly imaged area is the large pattern of rays that extend from the northern region of Mercury to regions south of Kuiper.”

From the Official Messenger site.

The Planetary Blog today posted an animation of Comet Halley captured by Vega 1 in 1986. The low quality of the Vega images reminded me of how low quality all the mission images to Halley were for their historic encounters. There was one image I found of Halley taken by Giotto that seemed to me to be the best I had ever seen in terms of detail and captured much of the coma that envelopes the nucleus as well. Here is that original image which was found at www.astro.lu.se.

The odd thing about it is the rarity of its use anywhere and the site that provided it gives no other detail about it other than “Nucleus of Comet Halley. Giotto fly-by 1986”. So out of curiosity, I decided to do a google image search for “Comet Halley” and turns out that the wallpaper image created by wanderingspace that features this image comes up first!

In the interest of full disclosure, I thought I would post the original to show how it was beautified. Most of the work was really cleaning up the noise and removing artifacts. Much of that noise was in the form of posterization and happens in the coma. So that noise was largely blurred out since the coma would pretty much just be a large blur of white at any rate, but the rate of gradation was still maintained for some level of legitimacy. Color was added to the image last, but that is entirely artistic. That and the upper left corner of the coma which was extended to fill the frame are the only fictional parts of the image.

All in all… it seems to me that when you remove the artifacts, you pretty much have the final image which was used for the wallpaper image. Less manipulation and more “clean-up” which is what I try to do with all images here when needed.

Asteroid Steins seen from a distance of around 800 km by Rosetta. This tiny asteroid is only around 5 km at it’s largest dimension with a crater on the top right that is approximately 1.5-km in size. That is a large impact for such a tiny body, but we have seen small bodies survive such large impacts before (Phobos, moon of Mars for instance). It seems like a pretty typical asteroid thus far and joins the growing family of such bodies visited by we humans. As a matter of fact, if I didn’t know where this came from — I would have assumed it was just another tiny moonlet imaged by Cassini in orbit around Saturn.

See the flyby animation on the official ESA Rosetta site. For those keeping score… the next major encounter in our Solar System is in just about a month with another Messenger visit to Mercury.

Steins, a rare E-type asteroid, is going to have company tomorrow as Rosetta swings by on its long voyage to Comet 67P/Churyumov-Gerasimenko scheduled to occur in 2014. See a quick computer simulation of tomorrow’s encounter here.

The encounter is to take place on Sept 5 with data and images to be communicated back to Earth that evening. Processing of that information is to take place on the 6th along with a press conference. Chances are, images and other information will not become public until that conference is underway as ESA still likes to roll things out the old fashioned way.

Here is an interesting comparison found on the Japanese Kaguya mission site. The two images shown above are of the Apollo 17 landing site. The top is obviously a photo taken on location by an Apollo astronaut and the lower image is a render from data taken by Kaguya in orbit around the moon. When programmers compile their data to show how the moon looks from the same position as the original Apollo photographer, the results come pretty close to matching. Such a comparison offers an idea of how real other such renders we may see from the mission can be trusted.

Nice color (close to natural) from July 14, 2005 by Gordan Ugarkovic. The resolution wasn’t very high, so this is as big as it gets.

On Cassini’s close shave of Enceladus it captured and image of what seems to be a strange tall mound of something at middle right. Look at how long a shadow it casts.

This is also in semi-false/true color using infrared, green and ultraviolet for RGB. Can you tell from its richness of color?!

I am no scientist, but I would think that the wispy soft lines billowing from this fracture on Enceladus are the famed geysers we have seen so much of from a distance (see the upper right side of the fracture in particular). The geysers have been easily seen from more distant and back-lit images taken of Enceladus, and we know this area being imaged is the source. So wouldn’t it be fairly safe to assume that it is happening in several of these frames?

It may just be that the particles are too fine to be seen at this distance. Consider that they previously have only visible at greater distances when the plumes are back-lit in low-light situations. Seeing this activity from this distance may be kind of like trying to see a cloud when you are already in it… only harder.

From around 1288 km. Looks like T minus 10 seconds to touch down!

From 1567 km.

From 2621 km.

Closest image returned so far. Lots of missing data on the right was duplicated to fill in the gaps. This results in the right side looking lower in resolution than the left.