Lunar and Planetary Conference / 1874.pdf
URL: https://ui.adsabs.harvard.edu/abs/2018LPI....49.1874E/abstract
From the dataset abstract
Jezero crater, with a diameter of 45 km, hosts two inlet channels of deltaic remnants along with an outlet channel and embraces hydrated minerals [1-5]. NE Syrtis (located just south of...
Source: Thermophysical Characterization of Jezero Crater and NE Syrtis, Mars
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Additional Information
Field | Value |
---|---|
Data last updated | September 16, 2021 |
Metadata last updated | September 16, 2021 |
Created | September 16, 2021 |
Format | unknown |
License | Creative Commons Attribution |
created | over 3 years ago |
id | effc1605-cc76-481a-8654-7b235a04af42 |
package id | 1390357a-d938-4b9a-9fc2-19e4e85e010e |
revision id | 6f3c9d7b-7947-4dca-8a79-8295ad4525a3 |
state | active |