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      AN ORGANIC COSMO-BAROMETER: DISTINCT PRESSURE AND TEMPERATURE EFFECTS FOR METHYL SUBSTITUTED POLYCYCLIC AROMATIC HYDROCARBONS

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      Journal: The Astrophysical Journal
      Publisher: IOP Publishing

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          Calibration of the ruby pressure gauge to 800 kbar under quasi-hydrostatic conditions

          H. Mao, J. Xu, P. M. Bell (1986)
          Article 0 comments Cited 838 times – based on 0 reviews     Review now
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            Organic compounds in carbonaceous meteorites.

            Mark Sephton (2002)
            The carbonaceous chondrite meteorites are fragments of asteroids that have remained relatively unprocessed since the formation of the solar system 4.6 billion years ago. These carbon-rich objects contain a variety of extraterrestrial organic molecules that constitute a record of chemical evolution prior to the origin of life. Compound classes include aliphatic hydrocarbons, aromatic hydrocarbons, amino acids, carboxylic acids, sulfonic acids, phosphonic acids, alcohols, aldehydes, ketones, sugars, amines, amides, nitrogen heterocycles, sulfur heterocycles and a relatively abundant high molecular weight macromolecular material. Structural and stable isotopic characteristics suggest that a number of environments may have contributed to the organic inventory, including interstellar space, the solar nebula and the asteroidal meteorite parent body. This review covers work published between 1950 and the present day and cites 193 references.
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              Hit-and-run planetary collisions.

              Erik Asphaug, Craig B Agnor, Quentin Williams (2006)
              Terrestrial planet formation is believed to have concluded in our Solar System with about 10 million to 100 million years of giant impacts, where hundreds of Moon- to Mars-sized planetary embryos acquired random velocities through gravitational encounters and resonances with one another and with Jupiter. This led to planet-crossing orbits and collisions that produced the four terrestrial planets, the Moon and asteroids. But here we show that colliding planets do not simply merge, as is commonly assumed. In many cases, the smaller planet escapes from the collision highly deformed, spun up, depressurized from equilibrium, stripped of its outer layers, and sometimes pulled apart into a chain of diverse objects. Remnants of these 'hit-and-run' collisions are predicted to be common among remnant planet-forming populations, and thus to be relevant to asteroid formation and meteorite petrogenesis.
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                Author and article information

                Journal
                Title: The Astrophysical Journal
                Abbreviated Title: ApJ
                Publisher: IOP Publishing
                ISSN (Print): 0004-637X
                ISSN (Electronic): 1538-4357
                Publication date Created: April 01 2014
                Publication date (Print): March 10 2014
                Volume: 784
                Issue: 2
                Page: 98
                Article
                DOI: 10.1088/0004-637X/784/2/98
                SO-VID: 70c218c5-f66c-4fca-9723-288947f07739
                Copyright © © 2014
                License:

                http://iopscience.iop.org/info/page/text-and-data-mining

                History

                Keywords: astrochemistry,FTIR spectroscopy,interplanetary medium,diamond anvil cell,high pressure
                Data availability:
                Keywords: astrochemistry, FTIR spectroscopy, interplanetary medium, diamond anvil cell, high pressure

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