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  1. A Martian meteorite is a rock that formed on Mars, was ejected from the planet by an impact event, and traversed interplanetary space before landing on Earth as a meteorite. As of September 2020 , 277 meteorites had been classified as Martian, less than half a percent of the 72,000 meteorites that have been classified.

  2. › wiki › MeteoriteMeteorite - Wikipedia

    • Fall Phenomena
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    Most meteoroids disintegrate when entering the Earth's atmosphere. Usually, five to ten a year are observed to fall and are subsequently recovered and made known to scientists. Few meteorites are large enough to create large impact craters. Instead, they typically arrive at the surface at their terminal velocityand, at most, create a small pit. Lar...

    Most meteorites are stony meteorites, classed as chondrites and achondrites. Only about 6% of meteorites are iron meteorites or a blend of rock and metal, the stony-iron meteorites. Modern classification of meteorites is complex. The review paper of Krot et al. (2007)summarizes modern meteorite taxonomy. About 86% of the meteorites are chondrites, ...

    In March 2015, NASA scientists reported that complex organic compounds found in DNA and RNA, including uracil, cytosine, and thymine, have been formed in the laboratory under outer space conditions, using starting chemicals, such as pyrimidine, found in meteorites. Pyrimidine and polycyclic aromatic hydrocarbons (PAHs) may have been formed in red g...

    Most meteorites date from the early Solar System and are by far the oldest extant material on Earth. Analysis of terrestrial weatheringdue to water, salt, oxygen, etc. is used to quantify the degree of alteration that a meteorite has experienced. Several qualitative weathering indices have been applied to Antarctic and desertic samples. The most co...

    A "meteorite fall", also called an "observed fall", is a meteorite collected after its arrival was observed by people or automated devices. Any other meteorite is called a "meteorite find". There are more than 1,100 documented falls listed in widely used databases, most of which have specimens in modern collections. As of January 2019[update], the ...

    Meteorites have figured into human culture since their earliest discovery as ceremonial or religious objects, as the subject of writing about events occurring in the sky and as a source of peril. The oldest known iron artifacts are nine small beads hammered from meteoritic iron. They were found in northern Egypt and have been securely dated to 3200...


    Meteorites are always named for the places they were found, where practical, usually a nearby town or geographic feature. In cases where many meteorites were found in one place, the name may be followed by a number or letter (e.g., Allan Hills 84001 or Dimmitt (b)). The name designated by the Meteoritical Societyis used by scientists, catalogers, and most collectors.

    Disintegrating meteoroids

    1. Tunguska event in Siberia1908 (no crater) 2. Vitim eventin Siberia 2002 (no crater) 3. Chelyabinsk eventin Russia 2013 (no known crater)

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  4. A meteorite resulting from 433 Eros would still be overall cold, because the heating effect probably drops to zero within the first centimeter depth. Also any existing ice would probably be safely stored in fluid inclusions. Regarding the first paragraph: You are right about that source being very anecdotal.

  5. › wiki › NakhliteNakhlite - Wikipedia

    A 2017 study dated them to at least four different eruptions from 1416 ± 7 Ma to 1322 ± 10 Ma. It has been shown that the nakhlites were suffused with liquid water around 620 million years ago and that they were ejected from Mars around 10.75 million years ago by an asteroid impact. They fell to Earth within the last 10,000 years.

  6. feldspathic regolith breccia; FIRST RECOGNISED LUNAR METEORITE. Yamato 82192/82193/86032. 1983–1986. 712. feldspathic fragmental breccia. EET 87521/96008. 1987–1996. 84. basaltic or gabbroic fragmental breccia.

  7. The 6.1 second fall of the Murrili meteorite was recorded by five Desert Fireball Network cameras. The rock entered the Earth's atmosphere at 13.82 km/s, and slowed to a speed of 3.83 km/s over 72 km, at an altitude of 18.34 km. The fall in dark flight was modeled using the WRF climate model to determine the final fall location

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