



NASA's beautiful collection of astromaterials is meticulously collected, catalogued and preserved for researchers to delve into the origins of our planet and the solar system
By Marissa Fessenden | August 8, 2012 | 9
While standing on the surface of the moon, Apollo 12 astronaut Alan Bean holds a lunar soil sample in a Special Environmental Sample Container....[More]
While standing on the surface of the moon, Apollo 12 astronaut Alan Bean holds a lunar soil sample in a Special Environmental Sample Container. Fellow astronaut Pete Conrad, Jr., is reflected in Bean's helmet visor. [Less] [Link to this slide]
The chalky, slightly crumbled piece of rock is a sample of ancient lunar crust. The device behind the rock shows the sample number and a scale....[More]
The chalky, slightly crumbled piece of rock is a sample of ancient lunar crust. The device behind the rock shows the sample number and a scale. The cube roughly shows the rock's orientation on the lunar surface—the side facing the camera was pointed north and the top of the rock was pointed up. The turntable lets scientists match the rock's orientation in the lab with shadow directions from its pictures on the moon's surface. [Less] [Link to this slide]
The dark glitter of a lunar meteorite stands out against the snow of Antarctica. Miller Range 05035 is a piece of the moon. Scientists analyzed the rock's age and composition and determined that it was ejected from the moon recently because of its old age—3.8 billion years—and oxygen isotope signature that is identical to Apollo samples....[More]
The dark glitter of a lunar meteorite stands out against the snow of Antarctica. Miller Range 05035 is a piece of the moon. Scientists analyzed the rock's age and composition and determined that it was ejected from the moon recently because of its old age—3.8 billion years—and oxygen isotope signature that is identical to Apollo samples. [Less] [Link to this slide]
Elephant Moraine A79001 is a Martian meteorite found in Antarctica's Elephant Moraine Ice Field in 1980. Black spheres embedded in the gray basaltic rack are capsules of glass containing trapped gas from the Martian atmosphere....[More]
Elephant Moraine A79001 is a Martian meteorite found in Antarctica's Elephant Moraine Ice Field in 1980. Black spheres embedded in the gray basaltic rack are capsules of glass containing trapped gas from the Martian atmosphere. Studies of noble gases and nitrogen trapped in these pockets matched the atmospheric composition measured by the NASA Viking mission in 1976. [Less] [Link to this slide]
This image may look like a stained-glass window, but it is actually a thin section of the Martian meteorite Miller Range 03346 taken in cross-polarized light....[More]
This image may look like a stained-glass window, but it is actually a thin section of the Martian meteorite Miller Range 03346 taken in cross-polarized light. Large crystals of clinopyroxene, a mineral often found in volcanic rocks, are surrounded by tiny shards of glass that have melted and recrystallized. The rock was likely formed in a shallow magma chamber on Mars about 1.3 billion years ago. [Less] [Link to this slide]
Dust from the Comet Wild 2 streaked through aerogel, a low-density silica-based material, on board the Stardust space probe, leaving this track....[More]
Dust from the Comet Wild 2 streaked through aerogel, a low-density silica-based material, on board the Stardust space probe, leaving this track. The Stardust mission was the first to collect and return cosmic dust and samples from a comet's tail. Magnified photographs of grains recovered from the track are inset in this image. [Less] [Link to this slide]
This interplanetary dust particle probably came from a comet before reaching Earth's upper stratosphere. One of NASA's high-flying aircraft collected the falling particle before it mixed with terrestrial dust....[More]
This interplanetary dust particle probably came from a comet before reaching Earth's upper stratosphere. One of NASA's high-flying aircraft collected the falling particle before it mixed with terrestrial dust. [Less] [Link to this slide]
A scientist carefully handles the Miller Range 07001 meteorite. Analysis reveals it has the same infrared spectrum as the asteroid Vesta, and contains the minerals pyroxene, olivine and chromite, which could have originated at the birth of the solar system, 4.56 billion years ago....[More]
A scientist carefully handles the Miller Range 07001 meteorite. Analysis reveals it has the same infrared spectrum as the asteroid Vesta, and contains the minerals pyroxene, olivine and chromite, which could have originated at the birth of the solar system, 4.56 billion years ago. [Less] [Link to this slide]
A researcher examines one of the collection arrays before it was attached to the Genesis spacecraft. The mission collected particles from solar wind....[More]
A researcher examines one of the collection arrays before it was attached to the Genesis spacecraft. The mission collected particles from solar wind. The hexagonal wafers are coated with thin layers of materials like silicon, geranium and gold-on-sapphire. [Less] [Link to this slide]
These researchers, suited to prevent sample contamination, are in a sample laboratory where scientists store and analyze solar wind particles collected during the Genesis spacecraft mission.
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This thin section shows the meteorite La Paz Ice Field 02228, found in Antarctica in 2002. It is a carbonaceous chondrite, a rock formed from dust and small grains only present in the early solar system....[More]
This thin section shows the meteorite La Paz Ice Field 02228, found in Antarctica in 2002. It is a carbonaceous chondrite, a rock formed from dust and small grains only present in the early solar system. The purple and blue circles are cross-sections of chondrules, originally a molten or partially molten droplet formed at high temperatures in the solar nebula. Chondrules are one of the oldest solids in the solar system. [Less] [Link to this slide]
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I've read references in both science and science-fiction articles to "asteroid mining." Is this a feasible thing to do? If so, how might it be accomplished, and what kind of valuable materials could we extract?
The Spirit of Exploration
Curiosity Rover Zeroes In on Traces of Past Habitats on Mars
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9 Comments
Add CommentRe: "About one in one thousand of the meteorites that fall on Earth was actually knocked off Mars by ancient impacts..."
Reply | Report Abuse | Link to thisThat claim has perplexed me since the days of the celebrated, "Allan Hills 84001 (commonly abbreviated ALH 84001),"
http://en.wikipedia.org/wiki/Allan_Hills_84001.
The alleged Martian location has been touted as, "...the Eos Chasma, a branch of the enormous Valles Marineris canyon system...The analysis, based on the rock's mineral characteristics, was presented by Vicky Hamilton of the University of Hawaii...the claim remains highly controversial..." http://www.newscientist.com/article/dn8004.
It raises the following question for me: What is the experimental evidence that an object can impact the martian surface with sufficient force to eject a meteorite on a trajectory to Earth?
The trajectory doesn't have to be Earth. As the rocks are scattered some may end up in Earth's path and are then vacuumed up by Earth's gravity. Mar's gravity is much weaker than Earth's so early impacts likely sent up many tonnes of material. Material from objects impacting with Earth have also been sent into space. We call it the moon.
Reply | Report Abuse | Link to thisRSchmidt,
Reply | Report Abuse | Link to thisThat explanation does not answer the question raised concerning experimental evidence as opposed to assertion. It does, however, raise another question: What objects impacting with Earth have been subsequently ejected onto the moon?
Cigarshaped,
Reply | Report Abuse | Link to this"How to Etch Your Own Crater" may be an interesting laboratory experiment. How does it provide an answer to my question?
@Bill_Crofut: I expect this derives from practical impact experiments with results scaled up to the planetary scale. Physics and fluid dynamics are good at this sort of thing.
Reply | Report Abuse | Link to thisBill, Your original question "What ..object can impact the martian surface with sufficient force to eject a meteorite ..?
Reply | Report Abuse | Link to thisMy first answer is that no OBJECT is needed to make direct contact. I doubt if more than a few % of craters were formed by IMPACT. The majority, which we now know pockmark every lump of rock out in the solar system, can only be the result of cosmic electrical interaction between these bodies. Just count how many circular craters also have raised central peaks. How many experiments can show impacts producing such neat shapes?
Watch my video and see the way plasma works. Twin rotating filaments of intense current etch away material in a spinning motion, like a forked corkscrew. Thus the centre is often left untouched. So if this 'mechanism' is applied to Valle Marineris you can see the symmetrial reversed 'S' shape resulting from a pair of massive discharge bolts of energy. w^3.holoscience.com/wp/wp-content/uploads/2012/03/Valmar_arc.jpg. Read the article at w^3.holoscience.com/wp/spiral-galaxies-grand-canyons/
Would you prefer to find a very big hammer and chizel to cut through 1" steel plate (impact)? Or would you switch on your super plasma cutting tool? The power is in the high currents possible when you are dealing with plasma in its 'arc' mode.
As you can see from the lab video, plasma naturally forms into intertwining filaments, known as Birkeland Currents. Since visible space is 99.99% plasma, the currents available in space are virtually unlimited. Making a gash the size of Valle Marineris is the job of a few minutes work. The excess material is lofted into space and all over the surface, as we can see from robot photos.
What agency or object caused this? A likely suspect, by the mythical records of humans around at the time, is Venus. The inexplicably hot and anti-rotating bad girl of ancient times, is very often referred to as a flaming comet. She was charged up and ready to zap! Astronomers treated her with awe and nations worshipped Baal, etc. Egypt worshipped her cometary form: w^3.gks.uk.com/comet-venus-velikovsky/
Tomato Addict,
Reply | Report Abuse | Link to thisThank you for that information. Have you a source for one or more of those experiments?
Cigarshaped,
Reply | Report Abuse | Link to thisUsing the “holoscience” entry you provided is a dead end. Revising it, i.e.,
http://www.holoscience.com/wp/wp-content/uploads/2012/03/Valmar_arc.jpg
does not lead to a video, but an image.
Revising the second entry, i.e.,
http://www.holoscience.com/wp/spiral-galaxies-grand-canyons/
does lead to the following web page:
“Spiral Galaxies & Grand Canyons.”
Please allow me some time to digest that information.
Cigarshaped,
Reply | Report Abuse | Link to thisHaving had the opportunity to read the online paper, “Spiral Galaxies & Grand Canyons,” one of the more significant statements for me is:
“No one was there to witness the evolution of the Earth, so geologists have constructed an elaborate story about the history of the Earth.”
You’ll bet no argument from me on that issue. However, how is your “Plasma Model” any different? For example,
“The missing mass (shades of the purely gravitational thinking of astronomers) was not transported or buried on Mars. It was lofted toward space by blast and electrical forces.”
How do you know that? How has your model been tested?