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55 cancri d in a sentence

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  • This eventually led to the discovery of the outer planet 55 Cancri d in 2002.
  • In the case of 55 Cancri d, this lower limit was around 3.835 times the mass of Jupiter.
  • Like the majority of known extrasolar planets, 55 Cancri d was detected by observing changes in its star's radial velocity.
  • A limitation of the radial velocity method used to discover 55 Cancri d is that only a lower limit on the planet's mass can be obtained.
  • Astrometric observations made with the Hubble Space Telescope suggest that the outer planet 55 Cancri d is inclined at 53?with respect to the plane of the sky.
  • Further astrometric observations with the Hubble Space Telescope on the outer planet 55 Cancri d suggest that planet is inclined at 53?to the plane of the sky; but innermost b and e are inclined at 85?
  • They honor the astronomers Nicolaus Copernicus, Galileo Galilei, Tycho Brahe and Thomas Harriot and the spectacle makers and telescope pioneers Jacharias Janssen . ( The IAU originally announced the winning name was Lippershey for 55 Cancri d.
  • Both the 43-day planet ( designated 55 Cancri c ) and the 5 AU planet ( designated 55 Cancri d ) were announced in the same paper, labeled in order of increasing distance from the star.
  • Assuming a composition similar to that of Jupiter and that the planet's atmosphere is close to chemical equilibrium, it is predicted that 55 Cancri d is covered in a layer of water clouds : the planet's internal heat probably keeps it too warm to form the ammonia-based clouds that are typical of Jupiter.
  • "' 55 Cancri d "'( abbreviated "'55 Cnc d "'), also named "'Lipperhey "', 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 our Sun, it is the fifth and outermost known planet in its planetary system . 55 Cancri d was discovered on June 13, 2002.
  • "' 55 Cancri d "'( abbreviated "'55 Cnc d "'), also named "'Lipperhey "', 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 our Sun, it is the fifth and outermost known planet in its planetary system . 55 Cancri d was discovered on June 13, 2002.
  • For instance, in the 55 Cancri system the first planet  55 Cancri b  was discovered in 1996; two additional farther planets were simultaneously discovered in 2002 with the nearest to the star being named 55 Cancri c and the other 55 Cancri d; a fourth planet was claimed ( its existence was later disputed ) in 2004 and named 55 Cancri e despite lying closer to the star than 55 Cancri b; and the most recently discovered planet, in 2007, was named 55 Cancri f despite lying between 55 Cancri c and 55 Cancri d.
  • For instance, in the 55 Cancri system the first planet  55 Cancri b  was discovered in 1996; two additional farther planets were simultaneously discovered in 2002 with the nearest to the star being named 55 Cancri c and the other 55 Cancri d; a fourth planet was claimed ( its existence was later disputed ) in 2004 and named 55 Cancri e despite lying closer to the star than 55 Cancri b; and the most recently discovered planet, in 2007, was named 55 Cancri f despite lying between 55 Cancri c and 55 Cancri d.
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