Astronomy:Kepler-277c
| Discovery | |
|---|---|
| Discovery site | Kepler Space Observatory |
| Discovery date | 2014 |
| Transit | |
| Orbital characteristics | |
| ~0.209 AU | |
| Eccentricity | null[1] |
| Orbital period | 33.006[1] d |
| Inclination | null[1] |
| Star | Kepler-277 |
| Physical characteristics | |
| Mean radius | 3.36 +0.83−0.72[1] R⊕ |
| Mass | 64.2 +18.1−15.7[1][2] M⊕ |
| Mean density | 9.33+15.33 −5.69 g cm−3 |
| 5.69+6.12 −2.93 g | |
| Physics | 745 K (472 °C; 881 °F)[3] |
Kepler-277c (also known by its Kepler Objects of Interest designation KOI-1215.02) is the third most massive and second-largest rocky planet ever discovered, with a mass about 64 times that of Earth. Discovered in 2014 by the Kepler Space Telescope, Kepler-277c is a Neptune-sized exoplanet with a very high mass and density for an object of its radius, suggesting a composition made mainly of rock with some amounts of water. Along with its sister planet, Kepler-277b, the planet's mass was determined using transit-timing variations (TTVs).
Characteristics
Size and temperature
Kepler-277c was detected using the transit method and TTVs, allowing for both its mass and radius to be determined to some level. It is approximately 3.36 R⊕, close to the size of Neptune. At that radius, most planets should be gaseous Mini-Neptunes with no solid surface. However, the mass of Kepler-277c is extremely high for its size. Transit-timing variations indicate a planetary mass of about 64.2 M⊕,[1] close to Saturn's mass at 95.16 M⊕. The planet has a density of approximately 9.33 g/cm3 and about 5.7 times the surface gravity of Earth. Such a high density for an object of this size implies that, like its sister planet, Kepler-277c is an enormous rock-based planet with a small portion of its mass as water.[2] It is currently the third most massive and second largest terrestrial planet ever discovered, behind Kepler-277b in mass[4] and PSR J1719-1438 b in both radius and mass.[5] Due to its proximity to its host star, Kepler-277c is quite hot with an equilibrium temperature of about 745 K (472 °C; 881 °F),[3] hot enough to melt certain metals.
Orbit
Kepler-277c orbits close to its host star, with one orbit lasting 33.006 days.[1] Its semi-major axis, or average distance from the parent object, is about 0.209 AU. For comparison, the planet Mercury takes 88 days to orbit the Sun at a distance of 0.38 AU. At this distance, Kepler-277c is very hot and most likely tidally locked to its host star. It is close to a 1:2 resonance with Kepler-277b, which orbits at an average distance of about 0.136 AU.
Host star
The parent star Kepler-277 is a large yellow star. It is 1.69 R☉ and 1.12 M☉, with a temperature of 5946 K, a metallicity of -0.315 [Fe/H], and an unknown age.[1] For comparison, the Sun has a temperature of 5778 K, a metallicity of 0.00 [Fe/H], and an age of about 4.5 billion years. The large radius in comparison to its mass and temperature suggest that Kepler-277 could be a Subgiant star.
See also
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 1.6 1.7 "Kepler-277 c CONFIRMED PLANET OVERVIEW PAGE". NASA Exoplanet Archive. https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-277+c&type=CONFIRMED_PLANET.
- ↑ 2.0 2.1 Xie, Ji-Wei (7 January 2014). "Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems". The Astrophysical Journal Supplement Series 210 (2): 25. doi:10.1088/0067-0049/210/2/25. Bibcode: 2014ApJS..210...25X.
- ↑ 3.0 3.1 "PHL's calculators". http://phl.upr.edu/projects/habitable-exoplanets-catalog/calculators.
- ↑ "Kepler-277". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/DisplayOverview/nph-DisplayOverview?objname=Kepler-277+b&type=CONFIRMED_PLANET.
- ↑ "A planet made of diamond". http://www.manchester.ac.uk/discover/news/a-planet-made-of-diamond/.
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