1 / 12

Jesús Martínez-Frías, Patrick McGuire & Javier Martin With the collaboration of

Centro de Astrobiología Near I-R spectroscopy experiment. Jesús Martínez-Frías, Patrick McGuire & Javier Martin With the collaboration of Javier Gómez-Elvira, Franck Selsis, Rafael Gomez-Blanco & Peter Jenniskens

colorado-lancaster
Download Presentation

Jesús Martínez-Frías, Patrick McGuire & Javier Martin With the collaboration of

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. Centro de Astrobiología Near I-R spectroscopy experiment Jesús Martínez-Frías, Patrick McGuire & Javier Martin With the collaboration of Javier Gómez-Elvira, Franck Selsis, Rafael Gomez-Blanco & Peter Jenniskens “...Spain is taking a leading role in this year's Leonid MAC mission. The Centro de Astrobiologia (CSIC/INTA) at Torrejon de Ardoz, near Madrid, will host the 2002 Leonid MAC deployment and participate key experiments on the DC-8 Airborne Laboratory. The Centro de Astrobiologia is a full partner of NASA's Astrobiology Institute...”http://leonid.arc.nasa.gov/

  2. METEORITES: acid-insoluble polymer, hydrocarbons, monocarboxylic acids, primary alcohols, aldehydes, ketones, amines, urea, purines, amino acids and carbonates. COMETS: H, C, O, CN, CH, OH, H2O+, CN+, CH+, OH+, N2+, CO+, CO2+ and complex organic molecules such as CH3CN, H2CO, and HCO

  3. The GIOTTO probe traversed Halley's comet at high speed and was able to record mass spectra of impacting dust particles. The majority of the dust grains were found to be largely carbonaceous, justifying the description "CHON" material from their elemental compositions. Fingerprints of organic matter were found in the trail of this 1999 Leonid fireball, which endured to 55 kilometers (34 miles) above Earth, much lower than most Leonid meteors.

  4. Laboratorio de Geología Planetaria Mineralogical and geochemical studies of meteorites Carbonaceous chondrites Allende meteorite Ordinary chondrites Cañellas, Olmedilla de Alarcón, Olivenza, Reliegos and Cangas de Onís meteorites Mesosiderites Vaca Muerta meteorite 2 cm

  5. N_02x5 N_02x20 N_02x50 D Olivine Laser-MicroRaman detection of carbon in the Allende carbonaceous chondrite (in collaboration with Prof. Fernando Rull) G

  6. Detection of carbon by Laser-micro Raman in ordinary chondrites (in collaboration with Mª J. Muñoz and F. Rull) RELIEGOS Piroxeno D G OLIVENZA Piroxeno Carbon?

  7. Laser-MicroRaman detection of calcite in the Vaca Muerta mesosiderite (in collaboration with Prof. Fernando Rull) calcite N_02x50

More Related