
Teegarden's Star b - Wikipedia
Teegarden’s Star is a low-mass red dwarf, with a mass of around 9 percent the mass of the Sun, and with a temperature of around 2,900 K (2,630 °C; 4,760 °F).
Teegarden's Star b Planet: Size, Mass, Gravity, Surface Temperature …
Mar 3, 2024 · Teegarden's Star, the cosmic guardian of Teegarden's Star b, is a low-mass red dwarf boasting only 9 percent of the Sun's mass. With a temperature around 2,900 Kelvin, this …
Teegarden’s Star revisited - arXiv.org
The FFD indicates that Teegarden’s Star may produce flares energetic enough for a planet with 1.08 Earth irradiation, such as planet b (Table 4), to enter the abiogenesis zone defined by …
Teegarden’s Star-b and c: Exoplanets Nearly as Good as Earth?
Feb 28, 2025 · It has an orbital period of Prot = 11.4 days, an approximate mass of Mp sin i ≈ 1.05 M, a bolometric irradiance of S/S ≈ 0.35, and an equilibrium temperature of Teq ≈ 263 K.
Teegarden’s Star b: (Almost) Too Hot to Handle? | astrobites
Nov 6, 2025 · The global mean surface temperature (top) and planetary albedo (bottom) of Planet b are shown with various installation values. The filled markers represent models that reached …
Teegarden’s Star b - NASA Science
Jul 7, 2025 · Teegarden's Star b is a super Earth exoplanet that orbits a M-type star. Its mass is 1.16 Earths, it takes 4.9 days to complete one orbit of its star, and is 0.0259 AU from its star.
Planet Teegarden's b
Detailed information about planet Teegarden's b and its parameters.
Near The Runaway: The Climate And Habitability Of Teegarden’s Star b
Oct 15, 2025 · We employ a suite of three-dimensional global climate model (GCM) simulations to (1) map the inner boundary of the habitable zone of Teegarden’s Star b and (2) characterize …
Report on Teegarden's Star b: Habitability Potential and
Liquid water The major factor is that the exoplanet Teegarden’s Star b orbits very closely to Teegarden’s Star (emits less light - Red Dwarf) in the habitable zone, where the surface …
Teegarden's Star b - Wikiwand
Teegarden’s Star is a low-mass red dwarf, with a mass of around 9 percent the mass of the Sun, and with a temperature of around 2,900 K (2,630 °C; 4,760 °F).