Results 31 to 40 of about 4,433 (297)
ASTROPHYSICAL PARAMETERS AND HABITABLE ZONE OF THE EXOPLANET HOSTING STAR GJ 581 [PDF]
, 2011 GJ 581 is an M dwarf host of a multiplanet system. We use long-baseline interferometric measurements from the CHARA Array, coupled with trigonometric parallax information, to directly determine its physical radius to be 0.299 ± 0.010 R_☉.
Kane, Stephen R. +43 more
core +1 more source
A Second Earth-sized Planet in the Habitable Zone of the M Dwarf, TOI-700 [PDF]
, 2023 We report the discovery of TOI-700 e, a 0.95 R _⊕ planet residing in the Optimistic Habitable Zone (HZ) of its host star. This discovery was enabled by multiple years of monitoring from NASA’s Transiting Exoplanet Survey Satellite (TESS) mission.
Kane, Stephen R. +63 more
core +1 more source
The Habitable Zone of Inhabited Planets [PDF]
, 2014 Abstract. In this paper we discuss and illustrate the hypothesis that life substantially alters the state of a planetary environment and therefore, modifies the limits of the HZ as estimated for an uninhabited planet. This hypothesis lead to the introduction of the Habitable Zone for Inhabited Planets (hereafter InHZ), defined here as the region where ...
Jorge I. Zuluaga +3 more
openaire +5 more sources
The Habitable-Zone Planet Finder: improved flux image generation algorithms for H2RG up-the-ramp data [PDF]
, 2018 Noise and stability of current state of the art near-infrared (NIR) array detectors are still substantially worse than optical science grade CCDs used in astronomy.
Ford, Eric B. +26 more
core +1 more source
No Transits of Proxima Centauri Planets in High-Cadence TESS Data
Frontiers in Astronomy and Space Sciences, 2021 Proxima Centauri is our nearest stellar neighbor and one of the most well-studied stars in the sky. In 2016, a planetary companion was detected through radial velocity measurements.
Emily A. Gilbert +9 more
doaj +1 more source
KRITERIA PLANET LAYAK HUNI SEBAGAI ANALISIS KEBERADAAN DOPPELGANGER BUMI
Gravity: Jurnal Ilmiah Penelitian dan Pembelajaran Fisika, 2019 The discovery of extrasolar planets has reached rapid development. Until now, various earth-sized planets called terrestrial planets around their parent stars have been discovered .
Berthianna Nurcresia +4 more
doaj +1 more source
Inner Habitable Zone Boundary for Eccentric Exoplanets
The Astrophysical Journal Letters, 2023 The climate of a planet can be strongly affected by its eccentricity due to variations in the stellar flux. There are two limits for the dependence of the inner habitable zone boundary (IHZ) on eccentricity: (1) the mean stellar flux approximation ( ${S ...
Xuan Ji +5 more
doaj +1 more source
Tides, planetary companions, and habitability: habitability in the habitable zone of low-mass stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2014 Earth-scale planets in the classical habitable zone (HZ) are more likely to be habitable if they possess active geophysics. Without a constant internal energy source, planets cool as they age, eventually terminating tectonic activity and rendering the planet sterile to life.
Van Laerhoven, Christa +2 more
openaire +2 more sources
A Catalog of Kepler Habitable Zone Exoplanet Candidates [PDF]
, 2016 International audienceThe NASA Kepler mission has discovered thousands of new planetary candidates, many of which have been confirmed through follow-up observations.
Ciardi, David R., +26 more
core +1 more source
Exomoons in the Habitable Zones of M Dwarfs [PDF]
The Astrophysical Journal, 2019 Abstract M dwarfs host most of the exoplanets in the local Milky Way. Some of these planets, ranging from sub-Earths to super-Jupiters, orbit in their stars’ habitable zones (HZs), although many likely possess surface environments that preclude habitability.
Héctor Martínez-Rodríguez +4 more
openaire +4 more sources