[meteorite-list] Meteorite Picture of the Day

2015-08-30 Thread Paul Swartz via Meteorite-list
Today's Meteorite Picture of the Day: La Grange

Contributed by: Anne Black

http://www.tucsonmeteorites.com/mpodmain.asp?DD=08/30/2015
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[meteorite-list] AD- No Reserve Lunars and more

2015-08-30 Thread Rob Wesel via Meteorite-list

Hello all

I have another auction run coming to an end in a few hours, great deals to 
be had on Lunar, CM2, irons


http://www.ebay.com/sch/nakhladog/m.html

Rob Wesel

Nakhla Dog Meteorites
www.nakhladogmeteorites.com
www.facebook.com/Nakhla.Dog.Meteorites
www.facebook.com/Rob.Wesel



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[meteorite-list] AD-Auctions Ending Today

2015-08-30 Thread mail--- via Meteorite-list
I have some auctions ending today including a fresh howardite with
flowlines, a complete 30g lunar, New Orleans, Shelburne, D'Orbigny,
Juvinas, and others. Please have a look here:

http://stores.ebay.com/Mile-High-Meteorites/

Thanks,
Matt Morgan
Mile High Meteorites
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[meteorite-list] Mars Rover Opportunity Update: Jul 21-30, 2015

2015-08-30 Thread Ron Baalke via Meteorite-list

OPPORTUNITY UPDATE: Beginning to Explore 'Marathon Valley',
sols 4085-4093, July 21, 2015-July 30, 2015

Opportunity has entered 'Marathon Valley' on the west rim of Endeavour 
Crater and has begun the search for clay minerals. 

Previously, the project tested returning to using Flash memory for data 
storage. The Flash exhibited instability after a few sols, so the project 
returned Opportunity to operating in RAM-only mode on Sol 4085 (July 21, 
2015). Over the next two sols a 360-degree Navigation Camera (Navcam) 
panorama was collected. 

On Sol 4088 (July 24, 2015), the rover resumed contact science with the 
collection of a Microscopic Imager (MI) mosaic of a surface target followed 
by the placement of the Alpha Particle X-ray Spectrometer (APXS) on the 
same for a multi-hour integration. Additional MI images were collected 
on the next sol to complete the mosaic. Atmospheric observations were 
also made as part of this multi-sol plan. 

On Sol 4091, (July 28, 2015), the Rock Abrasion Tool (RAT) was used to 
brush the surface target to prepare it for further investigation. This 
was followed by another MI mosaic and the placement of the APXS. On Sol 
4093 (July 30, 2015), an offset MI mosaic was collected and the APXS placed 
on the offset target. Other than the Flash, Opportunity is in good health. 

As of Sol 4092 (July 29, 2015), the solar array energy production was 
424 watt-hours with an atmospheric opacity (Tau) of 0.695 and a solar 
array dust factor of 0.611.

Total odometry is 26.40 miles (42.48 kilometers), more than a marathon.

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[meteorite-list] Dawn Journal - August 21, 2015

2015-08-30 Thread Ron Baalke via Meteorite-list

http://dawnblog.jpl.nasa.gov/2015/08/21/dawn-journal-august-21/

Dawn Journal 
by Dr. Marc Rayman
August 21, 2015

Dear Unhesidawntingly Enthusiastic Readers,

An ambitious explorer from Earth is gaining the best views ever of dwarf 
planet Ceres. More than two centuries after its discovery, this erstwhile 
planet is now being mapped in great detail by Dawn.

The spacecraft is engaged in some of the most intensive observations of 
its entire mission at Ceres, using its camera and other sensors to scrutinize 
the alien world with unprecedented clarity and completeness. At an average 
altitude of 915 miles (1,470 kilometers) and traveling at 400 mph (645 
kilometers per hour), Dawn completes an orbit every 19 hours. The pioneer 
will be here for more than two months before descending to its final orbit.

The complex spiral maneuver down from the second mapping orbit at 2,700 
miles (4,400 kilometers) went so well that Dawn arrived in this third 
mapping orbit on Aug. 13, which was slightly ahead of schedule. (Frequent 
progress of its descent, and reports on the ongoing work in the new orbit, 
are available here and on Twitter @NASA_Dawn.) It began this third mapping 
phase on schedule at 9:53:40 p.m. PDT on Aug. 17.
Map of Ceres with named craters

We had a detailed preview of the plans last year when Dawn was more than 
six thousand times farther from Ceres than it is today. (For reasons almost 
as old as Ceres itself, this phase is also known as the high altitude 
mapping orbit, or HAMO, although we have seen that it is the second lowest 
of the four mapping orbits.) Now let's review what will happen, including 
a change mission planners have made since then.

The precious pictures and other data have just begun to arrive on Earth, 
and it is too soon to say anything about the latest findings, but stand 
by for stunning new discoveries. Actually, you could get pictures about 
as good as Dawn's are now with a telescope 217 times the diameter of 
Hubble Space Telescope. An alternative is to build your own interplanetary 
spaceship, travel through the depths of space to the only dwarf planet 
in the inner solar system, and look out the window. Or go to the Ceres 
image gallery.

Dawn has already gained fabulous perspectives on this mysterious world 
from its first and second mapping orbits. Now at one third the altitude 
of the mapping campaign that completed in June, its view is three times 
as sharp. (Exploring the cosmos is so cool!) That also means each picture 
takes in a correspondingly smaller area, so more pictures are needed now 
to cover the entire vast and varied landscape. At this height, Dawn's 
camera sees a square about 88 miles (140 kilometers) on a side, less than 
one percent of the more than one million square miles (nearly 2.8 million 
square kilometers). The orbital parameters were chosen carefully so that 
as Ceres rotates on its axis every nine hours (one Cerean day), Dawn will 
be able to photograph nearly all of the surface in a dozen orbital loops.
his image, taken by NASA's Dawn spacecraft, shows the brightest spots 
on dwarf planet Ceres from an altitude of 2,700 miles (4,400 kilometers). 
The image, with a resolution of 1,400 feet (410 meters) per pixel, was 
taken on June 24, 2015.

When Dawn explored the giant protoplanet Vesta from comparable orbits 
(HAMO1 in 2011 and HAMO2 in 2012), it pointed its scientific instruments 
at the illuminated ground whenever it was on the dayside. Every time its 
orbit took it over the nightside, it turned to point its main antenna 
at Earth to radio its findings to NASA's Deep Space Network. As we explained 
last year, however, that is not the plan at Ceres, because of the failure 
of two of the ship's reaction wheels. (By electrically changing the 
speed at which these gyroscope-like devices rotate, Dawn can turn or stabilize 
itself in the zero-gravity conditions of spaceflight.)

We discussed in January that the flight team has excogitated innovative 
methods to accomplish and even exceed the original mission objectives 
regardless of the condition of the wheels, even the two operable ones 
(which will not be used until the final mapping orbit). Dawn no longer 
relies on reaction wheels, although when it left Earth in 2007, they were 
deemed indispensable. The spacecraft's resilience (which is a direct 
result of the team's resourcefulness) is remarkable!

One of the many ingredients in the recipe for turning the potentially 
devastating loss of the wheels into a solid plan for success has been 
to rotate the spacecraft less frequently. Therefore, sometimes Dawn will 
wait patiently for half an orbit (almost 9.5 hours) as it flies above 
ground cloaked in the deep darkness of night, its instruments pointed 
at terrain they cannot detect. Other times, it will keep its antenna fixed 
on Earth without even glancing at the sunlit scenery below, because it 
can capture the views on other revolutions. This strategy conserves hydrazine, 
the