Jump to content

File:My Pilgrimage to Meteorite Mecca (51104003032) (cropped).jpg

Page contents not supported in other languages.
This is a file from the Wikimedia Commons
From Wikipedia, the free encyclopedia

Original file (836 × 1,284 pixels, file size: 381 KB, MIME type: image/jpeg)

Summary

Description

with the leads from the ASU Center for Meteorite Studies, in its <a href="https://meteorites.asu.edu/cms60" rel="noreferrer nofollow">60th</a> year of operation, studying and classifying meteorites like forensic geologists spanning many world going back in time, even before our Earth formed. And they have a treasure trove of meteorites! I was like a kid in a candy shop when they opened the vault, and then the nitrogen filled storage bins with the rich organic emissaries from outer space.

They are actively studying the compositions of the most primitive classes of meteorites to better understand the time scales and processes involved in the formation of the first solid grains in the solar nebula, that eventually led to the formation of rocky planets like Earth and Mars. Meenakshi Wadhwa is the Director of the School of Earth and Space Exploration and will the the primary scientist for the Mars Sample Return Program (the 38 core samples to be obtained by the Perseverance rover). The techniques for meteoritic studies are quite relevant for sample returns of all types, whether from meteor, robot or human exploration.

I'm holding the fresh Aguas Zarcas CM2 fall from Costa Rica secured by Michael Farmer. Research Professor Laurence Garvie (right), in <a href="https://www.sciencemag.org/news/2020/08/unusual-meteorite-more-valuable-gold-may-hold-building-blocks-life" rel="noreferrer nofollow">Science</a>: "Aguas Zarcas is a carbonaceous chondrite, a pristine remnant of the early Solar System. It may hold amino acids, along with stardust that predates the Sun. Some scientists even believe rocks like Aguas Zarcas gave life a nudge when they crashed into a barren Earth 4.5 billion years ago."

Garvie uses high-spatial-resolution microscopy to study primitive chondritic meteorites as a means of understanding the physical and chemical processes that resulted in the formation of the Solar System. His particular field of interest is the relationship between organic and inorganic components in the carbonaceous chondrites, which can shed light on the abiotic processing of organic matter in the early Solar System.
Date
Source My Pilgrimage to Meteorite Mecca
Author Steve Jurvetson from Los Altos, USA
Other versions
image extraction process
This file has been extracted from another file
: My Pilgrimage to Meteorite Mecca (51104003032).jpg
original file

Licensing

w:en:Creative Commons
attribution
This file is licensed under the Creative Commons Attribution 2.0 Generic license.
You are free:
  • to share – to copy, distribute and transmit the work
  • to remix – to adapt the work
Under the following conditions:
  • attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.

Captions

Add a one-line explanation of what this file represents

Items portrayed in this file

depicts

6 April 2021

0.04 second

8.8 millimetre

image/jpeg

File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current13:04, 6 September 2021Thumbnail for version as of 13:04, 6 September 2021836 × 1,284 (381 KB)NearEMPTinessFile:My Pilgrimage to Meteorite Mecca (51104003032).jpg cropped 84 % horizontally, 54 % vertically using CropTool with lossless mode.

The following page uses this file:

Global file usage

The following other wikis use this file:

Metadata