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55 Cancri d (abbreviated 55 Cnc d), formally named Lipperhey / ˈ l ɪ p ər h iː /, is an extrasolar planet in a long-period orbit around the Sun-like star 55 Cancri A.Located at a similar distance from its star as Jupiter is from the Sun, it is the fifth and outermost known planet in its planetary system. 55 Cancri d was discovered on June 13, 2002.
The 55 Cancri system is located fairly close to the Solar System: the Gaia astrometry satellite measured the parallax of 55 Cancri A as 79.45 milliarcseconds, corresponding to a distance of 12.6 parsecs (41 light-years). [1] 55 Cancri A has an apparent magnitude of 5.95, making it just visible to the naked eye under very dark skies.
55 Cancri b is in a short-period orbit, though not so extreme as that of the previously detected hot Jupiter 51 Pegasi b.The orbital period indicates that the planet is located close to a 1:3 mean motion resonance with 55 Cancri c, however investigations of the planetary parameters in a Newtonian simulation indicate that while the orbital periods are close to this ratio, the planets are not ...
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55 Cancri f is located about 0.781 AU away from the star and takes 262 days to complete a full orbit. [10] A limitation of the radial velocity method used to detect 55 Cancri f is that only a minimum mass can be obtained, in this case around 0.144 times that of Jupiter, or half the mass of Saturn . [ 10 ]