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WebOct 13, 2012 · The universe just got a bit richer with the discovery of an apparent diamond -rich planet orbiting a nearby star. Dubbed 55 Cancri e, the rocky world is only twice the … The planet's transit of its host star was announced on 27 April 2011, based on two weeks of nearly continuous photometric monitoring with the MOST space telescope. The transits occur with the period (0.74 days) and phase that had been predicted by Dawson and Fabrycky. See more 55 Cancri e is an exoplanet in the orbit of its Sun-like host star 55 Cancri A. The mass of the exoplanet is about 8.63 Earth masses and its diameter is about twice that of the Earth, thus making it the first super-Earth discovered around a See more Like the majority of extrasolar planets found prior to the Kepler mission, 55 Cancri e was discovered by detecting variations in its star's radial velocity. This was achieved by … See more 55 Cancri e receives more radiation than Gliese 436 b. The side of the planet facing its star has temperatures more than 2,000 kelvin (approximately … See more • Jean Schneider (2011). "Notes for Planet 55 Cnc e". Extrasolar Planets Encyclopaedia. Retrieved 8 October 2011. • Spitzer Detects a Steaming Super-Earth Eclipsing Its Star (JPL 09.26.11) • Interactive visualisation of the 55 Cancri system See more In July 2014 the International Astronomical Union (IAU) launched NameExoWorlds, a process for giving proper names to certain exoplanets and their host stars. The process involved public nomination and voting for the new names. In December 2015, the IAU … See more The radial velocity method used to detect 55 Cancri e obtains the minimum mass of 7.8 times that of Earth, or 48% of the mass of Neptune. The transit shows that its inclination is about … See more • Appearance of extrasolar planets • Lists of exoplanets • Gliese 1132 b, the only other rocky exoplanet with a confirmed atmosphere. See more somany institute of technology \u0026 management
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