Skip to content
DraconiticResearch
Search Sources API
190,860 studies31 sourcesUpdated 23 min ago
PreprintCC BY 4.0HAL

The diversity of planetary climates in the Solar System as a basis for reflection and work on the study of exoplanet climates

Abstract

The main parameters allowing to characterize and compare the climatic features over the terrestrial planets of the Solar System are developed according to the distance from the host star; the existence of an atmosphere, its composition and motion; and the orbital parameters allowing to identify seasonal more or less contrasted oscillations (obliquity and eccentricity). The comparative climatology of the Solar System planets shows some common features subjected to many changes depending on different parameters of every planet. Like this, the rotation period (day/night duration), the obliquity and the eccentricity (seasonal oscillations) cause a wide variety of climatic conditions from a planet to an other one.

Related

  1. Diversity of planetary origins and compositions traced by stellar abundance differences among co-natal star systems
    Bertram Bitsch, Fan Liu, Haiyang S. Wang
    Astronomy & AstrophysicsPeer-reviewedPublisher termsSolar & stellar physicsCrossref
  2. Detailed study of HD 219134: A benchmark K dwarf with a compact planetary system
    J. Bétrisey, C. Pezzotti, G. Buldgen +4
    Astronomy & AstrophysicsPeer-reviewedPublisher termsSolar & stellar physicsCrossref
  3. Diversity of planetary origins and compositions traced by stellar abundance differences of co-natal star systems
    Bertram Bitsch, Fan Liu, Haiyang S. Wang
    arXivPreprintarXiv licenceFull textPlanetary science & exoplanetsSolar & stellar physicsarXiv
  4. Rescuing Kepler’s False Positives: A Possible Habitable Zone Exoplanet in the Triple-star System KOI-1623
    Rita Lanxuan 兰萱 Wang 王, Daniel Huber, Daniel Hey +6
    The Astronomical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
  5. Rescuing Kepler's False Positives: A Possible Habitable Zone Exoplanet in the Triple Star System KOI-1623
    Rita Lanxuan Wang, Daniel Huber, Daniel Hey +6
    arXivPreprintCC BY 4.0Full textPlanetary science & exoplanetsSolar & stellar physicsarXiv
BibTeX
@misc{planchon2026diversity,
  title = {{The diversity of planetary climates in the Solar System as a basis for reflection and work on the study of exoplanet climates}},
  author = {Olivier Planchon},
  howpublished = {HAL},
  year = {2026},
  month = sep,
  doi = {10.13140/rg.2.2.15747.05926},
  url = {https://hal.science/hal-05755387v1},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - The diversity of planetary climates in the Solar System as a basis for reflection and work on the study of exoplanet climates
AU  - Olivier Planchon
PY  - 2026
DA  - 2026/09/18
PB  - HAL
DO  - 10.13140/rg.2.2.15747.05926
UR  - https://hal.science/hal-05755387v1
AB  - The main parameters allowing to characterize and compare the climatic features over the terrestrial planets of the Solar System are developed according to the distance from the host star; the existence of an atmosphere, its composition and motion; and the orbital parameters allowing to identify seasonal more or less contrasted oscillations (obliquity and eccentricity). The comparative climatology of the Solar System planets shows some common features subjected to many changes depending on different parameters of every planet. Like this, the rotation period (day/night duration), the obliquity and the eccentricity (seasonal oscillations) cause a wide variety of climatic conditions from a planet to an other one.
ER  -