Phoenix Probe Lands on Mars

At 4:53:44 p.m. Pacific Time (7:53:44 p.m. Eastern Time) NASA’s Jet Propulsion Laboratory received radio signals from the Mars Phoenix Lander confirming that it survived its landing in the north polar region of Mars.

The probe enters the Martian atmosphere at about 78 miles above the surface and begins decelerating from its space cruise velocity of 12,500 miles per hour down to Mach 1.7 (1.7 times the speed of sound) when its parachute deployed.  The parachute is jettisoned at 1 km above the surface when the probe fires its rocket thrusters to decelerate it further until it reaches either 12 meters altitude or a speed of 5 miles per hour.  At this point the rocket engines stop and the probe drops to the surface.

Artist's Conception of Phoenix Probe 

Above is an artist’s conception.
I cant wait to see how it really will look!
Tomorrow…

Check the Phoenix Mission Site for updates!

Kevin Knuth
Albany NY

Posted under Astrobiology, Astronomy, Exploration, Mars, Robotics, Space

This post was written by drknuth on May 25, 2008

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Avalanche on Mars!

Avalanche on Mars! 

The Mars Reconnaissance Orbiter (MRO) captured for the first time ever an avalanche in progress on another world! 

Avalanche on Mars

These images were taken with the Hi Resolution Imaging Experiment (HiRISE) flying on the MRO.  This image was taken at 34° latitude and 235.8° longitude, which is in Mars’ north polar region. The geology of this region is that of a layered dome of material, and this cliff is located at the edge of it. The cliff is about one half of a mile high! (70 m = 2300 ft) and is incredibly steep with slopes as great as 60°.  The cloud of dust is about 590 feet across and extends about 625 feet from the base of the cliff.

This image was taken on February 18, 2008 at 1:05pm Martian local time. In the northern hemisphere of Mars, spring began on December 10, 2007, and the Carbon Dioxide ice (seen in the left side of the image at the top of the cliff) is beginning to thaw in the spring “heat”.  The Carbon Dioxide ice does not melt, instead it sublimes (turning from a solid to a gas).   As it does sediments and ice in these steep cliffs give way to avalanches. 

The scientists have been watching these particular locations with the hope of catching one in action.  They have succeeded!

Here you can compare before (PSP_007140_2640) and after (PSP_007338_2640) photos.

Kevin Knuth
Albany NY

Posted under Astronomy, Exploration, Mars, Space

This post was written by drknuth on March 11, 2008

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Large Asteriod May Collide with Mars

Orbit Diagram of 2007WD5 

There is now a 4 percent chance that the large asteriod 2007 WD5 may collide with the planet Mars in January 2008.  While there is a 96% chance that the asteriod will miss, these odds are much larger than usual for large asteriod impacts.  If the impact is to occur, it will be on 2008 January 30 at 10:56 UT (2:56 a.m. PST) +- a few minutes.

If this asteriod were heading toward Earth, we would be worried.  The fact that it may hit Mars provides a potential scientific opportunity to monitor a large impact on a terrestrial world from the several space probes currently orbiting Mars, or from the ground-based rovers.  The event would be comparable to the impact of Comet Shoemaker-Levy 9 on Jupiter in July 1994.

The asteriod, which was discovered on November 20, 2007 by the NASA-funded Catalina Sky Survey, recently passed the Earth at a distance of 5 million miles and is currently heading toward Mars at a speed of 27,900 miles per hour.  If a collision were to occur, it will produce a crater similar in size to Barringer Meteor Crater in Arizona with a blast of about 10-15 megatons of TNT, which is similar to the Tunguska Airburst in 1908.

The Near-Earth Object Program at NASA’s Jet Propulsion Laboratory monitors the orbits of known large near-Earth asteroids.  Here are two of their articles on this potential collision.

http://neo.jpl.nasa.gov/news/news153.html
http://neo.jpl.nasa.gov/news/news151.html

Kevin Knuth
Albany NY

Posted under Astronomy, Mars, Research, Space

This post was written by drknuth on December 28, 2007

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Martian Spiders, Lizard Skin and Lacework

 Mars Spider

While much of Mars looks like the deserts of Utah, the Martian South Polar regions have revealed some surprising geology unlike anything we have here on Earth.

At the 2007 American Geophysical Union Fall Meeting in San Francisco, Chris Okubo, Candace Hansen, and Timothy Titus who work with the Mars Reconnaissance Orbiter’s High Resolution Imaging Camera presented research suggesting that these intriguing structures are caused by explosions of subliming carbon dioxide.

Mars Spiders

The theory is that there is a layer of translucent Carbon Dioxide ice and when the surface is heated during the summer months, the ground beneath the ice heats up vaporizing the Carbon Dioxide gas.  This gas flows uphill and bursts out of weak spots in the ice.  This results in geysers which spew Carbon Dioxide gas and Martian dust into the atmosphere.  The gas refreezes and snows out forming the white material along the spider-shaped network of tunnels blown out by the subliming Carbon Dioxide.

Martian Lace

This same process is believed to be responsible for similar more extensive landscapes called lacework and lizard skin.  It would be fascinating to see these from the ground.

Kevin Knuth
Albany NY 

Posted under Astronomy, Exploration, Mars, Space

This post was written by drknuth on December 15, 2007

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Animations

I have made some animated gifs that I am putting on this blog’s Animations page.

This is an animation of a rotating Earth, and was constructed from 48 images generated by Celestia.  These were then stitched together and optimized using Adobe ImageReady.

Please feel free using these on your own website.
Just remember, they are not for sale or re-sale.
And stop back periodically because I will make more.

Enjoy,
Kevin Knuth
Albany NY

Posted under Astronomy, Climate, Fun, Green, Internet

This post was written by drknuth on November 22, 2007

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