[meteorite-list] Caught For The First Time: The Early Flash Of An Exploding Star

2016-03-23 Thread MexicoDoug via Meteorite-list
Haven't seen this covered by Ron.  Maybe not like I expected but in our 
lifetimes!  Look what K2/Kepler is reporting!  They caught the moment -actually 
about 20 minutes- that a star goes supernova, *visibly*, twice.  Wow, 
meticulous persistence pays.  Tycho Brahe would be so impressed...  They go on 
to say expanding brightness reaches a maximum after 14 days, as all the 
elements (like iron and nickel) are manufactured and released that make life 
and geology (and nice pre-stellar nebulae) interesting:

abstract:
http://arxiv.org/abs/1603.05657

preprint pdf:
http://arxiv.org/pdf/1603.05657v1.pdf

NASA PR Summary:
http://www.nasa.gov/feature/ames/Kepler/caught-for-the-first-time-the-early-flash-of-an-exploding-star

Caught For The First Time: The Early Flash Of An Exploding Star

The brilliant flash of an exploding star’s shockwave—what astronomers call the 
“shock breakout”—has been captured for the first time in the optical wavelength 
or visible light by NASA's planet-hunter, the Kepler space telescope.

An international science team led by Peter Garnavich, an astrophysics professor 
at the University of Notre Dame in Indiana, analyzed light captured by Kepler 
every 30 minutes over a three-year period from 500 distant galaxies, searching 
some 50 trillion stars. They were hunting for signs of massive stellar death 
explosions known as supernovae.
The brightness of a Type II supernova shock breakout
The diagram illustrates the brightness of a supernova event relative to the sun 
as it unfolds. For the first time, a supernova shockwave has been observed in 
the optical wavelength or visible light as it reaches the surface of the star. 
This early flash of light is called a shock breakout. The explosive death of 
this star, called KSN 2011d, as it reaches its maximum brightness takes 14 
days. The shock breakout itself lasts only about 20 minutes, so catching the 
flash of energy is an investigative milestone for astronomers. The unceasing 
gaze of NASA's Kepler space telescope allowed astronomers to see, at last, this 
early moment as the star blows itself to bits. Supernovae like these — known as 
Type II — begin when the internal furnace of a star runs out of nuclear fuel 
causing its core to collapse as gravity takes over. This type of star is called 
a red supergiant star and it is 20,000 times brighter than our sun. As the 
supergiant star goes supernova, the energy traveling from the core reaches the 
surfaces with a burst of light that is 130,000,000 times brighter than the sun. 
The star continues to explode and grow reaching maximum brightness that is 
about 1,000,000,000 times brighter than the sun.
Credits: NASA Ames/W. Stenzel

In 2011, two of these massive stars, called red supergiants, exploded while in 
Kepler’s view. The first behemoth, KSN 2011a, is nearly 300 times the size of 
our sun and a mere 700 million light years from Earth. The second, KSN 2011d, 
is roughly 500 times the size of our sun and around 1.2 billion light years 
away.

“To put their size into perspective, Earth's orbit about our sun would fit 
comfortably within these colossal stars,” said Garnavich.

Whether it’s a plane crash, car wreck or supernova, capturing images of sudden, 
catastrophic events is extremely difficult but tremendously helpful in 
understanding root cause. Just as widespread deployment of mobile cameras has 
made forensic videos more common, the steady gaze of Kepler allowed astronomers 
to see, at last, a supernova shockwave as it reached the surface of a star. The 
shock breakout itself lasts only about 20 minutes, so catching the flash of 
energy is an investigative milestone for astronomers.

“In order to see something that happens on timescales of minutes, like a shock 
breakout, you want to have a camera continuously monitoring the sky,” said 
Garnavich. “You don’t know when a supernova is going to go off, and Kepler's 
vigilance allowed us to be a witness as the explosion began.”

Supernovae like these — known as Type II — begin when the internal furnace of a 
star runs out of nuclear fuel causing its core to collapse as gravity takes 
over.

The two supernovae matched up well with mathematical models of Type II 
explosions reinforcing existing theories. But they also revealed what could 
turn out to be an unexpected variety in the individual details of these 
cataclysmic stellar events.

While both explosions delivered a similar energetic punch, no shock breakout 
was seen in the smaller of the supergiants. Scientists think that is likely due 
to the smaller star being surrounded by gas, perhaps enough to mask the 
shockwave when it reached the star's surface.

“That is the puzzle of these results,” said Garnavich. “You look at two 
supernovae and see two different things. That’s maximum diversity.”

Understanding the physics of these violent events allows scientists to better 
understand how the seeds of chemical complexity and life itself have been 
scattered in space and time in 

[meteorite-list] NASA Sends Fire, Meteor Experiments to International Space Station on Commercial Cargo Spacecraft

2016-03-23 Thread Ron Baalke via Meteorite-list

March 23, 2016

RELEASE 16-036

NASA Sends Fire, Meteor Experiments to International Space Station on 
Commercial Cargo Spacecraft

Scientific investigations of fire in microgravity and grippers inspired by 
geckos are among the nearly 7,500 pounds of cargo headed to the International 
Space Station aboard an Orbital ATK Cygnus spacecraft, along with equipment 
to support some 250 other experiments and studies aboard the world's only 
orbital laboratory.

Orbital ATK's fifth cargo delivery flight under its Commercial Resupply 
Services contract with NASA launched at 11:05 p.m. EDT Tuesday on a United 
Launch Alliance Atlas V rocket from Space Launch Complex 41 on Cape Canaveral 
Air Force Station in Florida. The Cygnus is scheduled to arrive at the 
orbiting laboratory Saturday, March 26.

The station's Expeditions 47 and 48 crews will employ these science 
payloads to support experiments in biology, biotechnology, physical science 
and Earth science - research that improves life on Earth -- including:

 * Saffire-I provides a new way to study a large fire on an exploration
   craft, which has not been possible in the past because the risks for
   performing such studies on spacecraft with astronauts aboard are too high.
 * Meteor will enable the first space-based observations of meteors
   entering Earth's atmosphere from space.
 * Strata-I could give us answers about how regolith behaves and moves in
   microgravity, how easy or difficult it is to anchor a spacecraft in
   regolith, how it interacts with spacecraft and spacesuit materials, and
   other important properties.
 * The Gecko Gripper study tests a gecko-inspired adhesive gripping
   device that can stick on command in the harsh environment of space.
 * The Additive Manufacturing Facility will add an upgraded 3-D printing
   capability to the station.

NASA astronaut and Expedition 46 Commander Tim Kopra will capture Cygnus at 
about 6:40 a.m. Saturday, March 26, using the space station's Canadarm2 
robotic arm to take hold of the spacecraft. Astronaut Tim Peake of ESA 
(European Space Agency) will support Kopra in a backup position. NASA TV 
coverage of capture will begin at 5:30 a.m.

Saffire-1 will remain on the spacecraft once all the other supplies are 
unloaded, and the vehicle will be attached to the space station for about two 
months. Once it departs and the spacecraft is a safe distance from the space 
station, engineers will remotely conduct the first Saffire experiment before 
the Cygnus' destructive reentry into Earth's atmosphere. Before detaching 
from the station, Cygnus will also be filled with about 3,000 pounds of 
trash, which will be burned up over the Pacific Ocean.

This is the second flight of an enhanced Cygnus spacecraft, and the second 
using the Atlas V launch system. The cargo freighter features a greater 
payload capacity, supported by new fuel tanks and solar arrays, and an 
extended pressurized cargo module that increases the spacecraft's interior 
volume by 25 percent, enabling more cargo to be delivered with each launch.

The space station is a convergence of science, technology and human 
innovation that demonstrates new technologies and makes research 
breakthroughs not possible on Earth. The space station has been continuously 
occupied since November 2000. In that time, it has been visited by more than 
200 people and a variety of international and commercial spacecraft. The 
space station remains the springboard to NASA's next great leap in 
exploration, including future missions to an asteroid and Mars.

For more information about Orbital ATK's mission, visit:

http://www.nasa.gov/orbitalatk

For more information about the International Space Station, visit:

http://www.nasa.gov/station

-end-


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[meteorite-list] MRO HiRISE Images: March 23, 2016

2016-03-23 Thread Ron Baalke via Meteorite-list


MARS RECONNAISSANCE ORBITER HIRISE IMAGES
March 23, 2016

o Stratigraphy of Alluvial Fans in Saheki Crater
  http://hirise.lpl.arizona.edu/ESP_044491_1585

  Some of the best-preserved alluvial fans on Mars are in 
  this area, which we've images many times previously.

o Old Salt
  http://hirise.lpl.arizona.edu/ESP_044502_1735

  Just what is that "purplish" colored stuff with the polygonal 
  fractures?

o Looking for Ice 
  http://hirise.lpl.arizona.edu/ESP_044698_2245

  At high latitudes, new impact craters often expose ice, which 
  appears bright in HiRISE enhanced-color images.

o Colorful Polar Layered Deposits
  http://hirise.lpl.arizona.edu/ESP_044706_2670

  The North Polar layered deposits provide a record of recent climate 
  changes on Mars.
 
All of the HiRISE images are archived here:

http://hirise.lpl.arizona.edu/

Information about the Mars Reconnaissance Orbiter is 
online at http://www.nasa.gov/mro. The mission is 
managed by NASA's Jet Propulsion Laboratory, a division 
of the California Institute of Technology, for the NASA 
Science Mission Directorate, Washington, D.C. Lockheed 
Martin Space Systems, of Denver, is the prime contractor 
and built the spacecraft. HiRISE is operated by the 
University of Arizona. Ball Aerospace and Technologies 
Corp., of Boulder, Colo., built the HiRISE instrument.

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Re: [meteorite-list] Tissint '2' classification

2016-03-23 Thread Bigjohn Shea via Meteorite-list
This is Tissint II.
Don't ask me how to pronounce it.  ;-)
http://www.lpi.usra.edu/meteor/metbull.php?code=62802

Sent using the mail.com mail app

On 3/23/16 at 2:47 PM, Kevin Kichinka via Meteorite-list wrote:

> Team Meteorite:
> 
> This 2015 fall seems not yet to have been classifiedor has it?
> 
> Kevin Kichinka
> mars...@gmail.com
> 'The Art of Collecting Meteorites' available on Amazon.com
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> 
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> Archives at http://www.meteorite-list-archives.com
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[meteorite-list] Tissint '2' classification

2016-03-23 Thread Kevin Kichinka via Meteorite-list
Team Meteorite:

This 2015 fall seems not yet to have been classifiedor has it?

Kevin Kichinka
mars...@gmail.com
'The Art of Collecting Meteorites' available on Amazon.com
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[meteorite-list] Meteor Experiment: Out the Window Looks from the Space Station

2016-03-23 Thread Leonard David via Meteorite-list



Meteor Experiment: Out the Window Looks from the Space Station


http://www.leonarddavid.com/meteor-experiment-out-the-window-looks-from-the-space-station/
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[meteorite-list] Wanted: pallasite peridots rough

2016-03-23 Thread matija bericic via Meteorite-list
Dear list,
Does anybody has pallasite peridots for sale? What I am looking for:
as gemmy as possible, rough (uncut), extracted from pallasite
(meteorite, ET origin) of course, all kinds of sizes and shapes. Pics
and prices please.
Is there anybody out there who has a knowledge how to extract peridots
from pallasite meteorite?
Thank you,
Matija
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[meteorite-list] Meteorite Picture of the Day

2016-03-23 Thread Paul Swartz via Meteorite-list
Today's Meteorite Picture of the Day: Zagami

Contributed by: Tomasz Jakubowski

http://www.tucsonmeteorites.com/mpodmain.asp?DD=03/23/2016
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