
Gliese 581 - Wikipedia
Gliese 581 (/ ˈɡliːzə /) is a red dwarf star of spectral type M3V which hosts a planetary system, 20.5 light-years (6.3 parsecs) away from Earth in the constellation Libra.
[2003.14314] NGTS J214358.5-380102 -- NGTS discovery of the …
2020年3月31日 · Spectral analysis of the system suggests a primary of spectral type M3V, consistent with both modelled masses and radii, and with SED fitting of NGTS photometry. As …
NTRS - NASA Technical Reports Server
The M3V dwarf star L 98-59 hosts three small (R < 1.6 Rꚛ) planets. The host star is bright (K = 7.1) and nearby (10.6 pc), making the system a prime target for follow-up characterization with …
Transit Timing Variations in the three-planet system: TOI-270
2023年8月21日 · Abstract: We present ground and space-based photometric observations of TOI-270 (L231-32), a system of three transiting planets consisting of one super-Earth and two sub …
(PDF) L 98-59: A Benchmark System of Small Planets for Future ...
2021年10月1日 · PDF | The M3V dwarf star L 98-59 hosts three small (R < 1.6 R ⊕) planets. The host star is bright (K = 7.1) and nearby (10.6 pc), making the system a... | Find, read and cite …
[2106.00685] L 98-59: a Benchmark System of Small Planets for …
2021年6月1日 · Abstract: L 98-59 is an M3V dwarf star that hosts three small (R < 1.6 Earth radii) planets. The host star is bright (K = 7.1) and nearby (10.6 pc), making the system a prime …
Title: Debris disks around M dwarfs: The Herschel DEBRIS survey
2025年2月6日 · In the M-dwarf subsample, two debris disks have been detected, around the M3V dwarf GJ581 and the M4V dwarf FomalhautC (LP876-10). This result gives a disk detection …
L 98-59: a Benchmark System of Small Planets for Future …
2021年6月1日 · L 98-59 is an M3V dwarf star that hosts three small (R < 1.6 Earth radii) planets. The host star is bright (K = 7.1) and nearby (10.6 pc), making the system a prime target for...
L 98-59: A Benchmark System of Small Planets for Future …
L 98-59 is an M3V dwarf star that hosts at least four small planets, three of which transit. The host star is bright and nearby, making the system a prime target for follow-up characterization. This …
Jup orbiting the M3V star HIP 79431. This is the sixth giant planet to be detected in Doppler surveys of M dwarfs and it is one of the most massive planets discovered around an M dwarf …
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