PRETHARSIS Virtual Observatory Resource

Authors
  1. Azria Chloe
  2. Published by
    IPSL/GEOPS
Abstract
 "The growth of the Tharsis volcanic complex on Mars during
Noachian/Hesperian era induced a reorientation of the spin axis of the
planet (true polar wander). This service gives access to a map of Mars
topography before Tharsis formation (Early Noachian) and a map of Mars
topography before true polar wander (Late Noachian/Early Esperian),
from the model described in Bouley, S., Baratoux, D., Matsuyama, I. et
al. Late Tharsis formation and implications for early Mars. Nature
531, 344–347 (2016). https://doi.org/10.1038/nature17171 ."
Keywords
  1. solar-system-astronomy
  2. planetary-science
  3. solar-system-planets
  4. solar-system-terrestrial-planets
  5. mars
  6. planetary-science
  7. planetary-surfaces
  8. planetary-structure
  9. surface-variability
Bibliographic source
Dataset DOI: 10.14768/20181024001.1 ; http://dx.doi.org/10.14768/20181024001.1
See also HTML
https://dachs-vo.ipsl.fr/tableinfo/pretharsis.epn_core
IVOA Identifier IVOID
ivo://geops.ipsl/pretharsis/q/epn_core

Access

IVOA Table Access TAP
https://dachs-vo.ipsl.fr/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2021-08-23T00:00:00Z
Resource record created
2024-05-17T01:18:57Z
updated

Contact

Name
Bouley Sylvain
Postal Address
GEOPS, batiment 339 Rue du Belvedere Campus Universitaire d'Orsay 91400 Orsay
E-Mail
sylvain.bouley@universite-paris-saclay.fr