Early Results from the HUMDRUM Survey: A Small, Earth-mass Planet Orbits TOI-1450A

M-dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUnting for M Dwarf Rocky planets Using MAROON-X (HUMDRUM) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precise masses of a volume-limited (

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Veröffentlicht in:	The Astronomical journal 2024-08, Vol.168 (2), p.67
Hauptverfasser:	Brady, Madison, Bean, Jacob L., Seifahrt, Andreas, Kasper, David, Luque, Rafael, Stefánsson, Guđmundur, Stürmer, Julian, Charbonneau, David, Collins, Karen A., Doty, John P., Essack, Zahra, Fukui, Akihiko, Grau Horta, Ferran, Hedges, Christina, Hellier, Coel, Jenkins, Jon M., Narita, Norio, Quinn, Samuel N., Shporer, Avi, Schwarz, Richard P., Seager, Sara, Stassun, Keivan G., Striegel, Stephanie, Watkins, Cristilyn N., Winn, Joshua N., Zambelli, Roberto
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Companion stars Density Dwarf planets Dwarf stars Earth Earth rotation Extrasolar planets Extrasolar rocky planets Extreme high temperatures Hunting M dwarf stars Planet detection Planetary composition Planetary orbits Planetary rotation Planets Public transportation Red dwarf stars Stars Terrestrial planets Transit
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Zusammenfassung:	M-dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUnting for M Dwarf Rocky planets Using MAROON-X (HUMDRUM) survey uses the MAROON-X spectrograph, which is ideally suited to studying these stars, to measure precise masses of a volume-limited (
ISSN:	0004-6256 1538-3881
DOI:	10.3847/1538-3881/ad500a