Recipes for forming a carbon–rich giant planet

O Mousis, T Cavalié, JI Lunine, KE Mandt… - Space Science …, 2024 - Springer
The exploration of carbon-to-oxygen ratios has yielded intriguing insights into the
composition of close-in giant exoplanets, giving rise to a distinct classification: carbon-rich …

Ideas for citizen science in astronomy

PJ Marshall, CJ Lintott… - Annual Review of …, 2015 - annualreviews.org
We review the expanding, internet-enabled, and rapidly evolving field of citizen astronomy,
focusing on research projects in stellar, extragalactic, and planetary science that have …

[HTML][HTML] Mid-infrared mapping of Jupiter's temperatures, aerosol opacity and chemical distributions with IRTF/TEXES

LN Fletcher, TK Greathouse, GS Orton, JA Sinclair… - Icarus, 2016 - Elsevier
Global maps of Jupiter's atmospheric temperatures, gaseous composition and aerosol
opacity are derived from a programme of 5–20 µm mid-infrared spectroscopic observations …

Changes in Jupiter's zonal wind profile preceding and during the Juno mission

J Tollefson, MH Wong, I de Pater, AA Simon, GS Orton… - Icarus, 2017 - Elsevier
We present five epochs of WFC3 HST Jupiter observations taken between 2009–2016 and
extract global zonal wind profiles for each epoch. Jupiter's zonal wind field is globally stable …

[HTML][HTML] Formation of jets and equatorial superrotation on Jupiter

T Schneider, J Liu - Journal of the atmospheric sciences, 2009 - journals.ametsoc.org
Formation of Jets and Equatorial Superrotation on Jupiter in: Journal of the Atmospheric
Sciences Volume 66 Issue 3 (2009) Jump to Content Jump to Main Navigation Logo Logo Logo …

[图书][B] Giant planets of our solar system: atmospheres, composition, and structure

P Irwin - 2009 - books.google.com
This book reviews the current state of knowledge of the atmospheres of the giant gaseous
planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are …

Atmospheric circulation of exoplanets

AP Showman, JYK Cho, K Menou - Exoplanets, 2010 - books.google.com
We survey the basic principles of atmospheric dynamics relevant to explaining existing and
future observations of exoplanets, both gas giant and terrestrial. Given the paucity of data on …

Deep winds beneath Saturn's upper clouds from a seasonal long-lived planetary-scale storm

A Sánchez-Lavega, T Río-Gaztelurrutia, R Hueso… - Nature, 2011 - nature.com
Convective storms occur regularly in Saturn's atmosphere,,,. Huge storms known as Great
White Spots, which are ten times larger than the regular storms, are rarer and occur about …

Storms and the depletion of ammonia in Jupiter: II. Explaining the Juno observations

T Guillot, C Li, SJ Bolton, ST Brown… - Journal of …, 2020 - Wiley Online Library
Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several
puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars …

Jupiter's temperate belt/zone contrasts revealed at depth by Juno microwave observations

LN Fletcher, FA Oyafuso, M Allison… - Journal of …, 2021 - Wiley Online Library
Juno microwave radiometer (MWR) observations of Jupiter's midlatitudes reveal a strong
correlation between brightness temperature contrasts and zonal winds, confirming that the …