Gamma Cephei oor Spaans

Gamma Cephei

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Errai

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As of early 2011 about 30 Jupiter class planets have been found around evolved K-giant stars including Pollux, Gamma Cephei and Iota Draconis.
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"But planets would be expected to be much rarer in systems like Gamma Cephei that have close companion stars.
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Infrared images of the gamma Cephei system obtained from Calar alto on September the 11th (left) and 12th (right) 2006.
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Astronomers have been left with no choice but to propose that a planet orbits the main star in the Gamma Cephei binary.
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The 5th magnitude stars are all variables: one (NV Puppis) is a Gamma Cassiopeiae variable, and the other (NW Puppis) is a Beta Cephei variable.
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Gamma Cephei Ab: The radial velocity variations of the star Gamma Cephei were announced in 1989, consistent with a planet in a 2.5-year orbit.
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1988–1994Edit Gamma Cephei Ab: The radial velocity variations of the star Gamma Cephei were announced in 1989, consistent with a planet in a 2.5-year orbit.
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Omega-Cass observations of gamma Cephei A+B (418 Kb) Infrared images of the gamma Cephei system obtained from Calar alto on September the 11th (left) and 12th (right) 2006.
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In 1988, they thought they had found evidence for a Jupiter in orbit around Gamma Cephei, but after taking more data, in 1992 they published a retraction of the claim.
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Residuals of the observed radial velocity of Errai (gamma Cephei) for almost 90 consecutive days (upper box) were obtained during autumn 2014. The one day zoom shows clearly the stellar oscillations.
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19 External links 1988–1992[edit] Gamma Cephei Ab: The radial velocity variations of the star Gamma Cephei were announced in 1989, consistent with a planet in a 2.5-year orbit.
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One of their recent findings refers to a quite bright star, gamma Cephei (Cephei Ab) with a minimum mass 1.7 times that of planet Jupiter and with a period of around 3 years.
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At the moment, if they existed extraterrestrial, we say, in some planet in the orbit of the star Gamma Cephei, to 48 distance year-light, only in 1984 they would receive the first original signals of emitted TELES of the Earth in 1936.
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13 sinne gevind in 6 ms. Hulle kom uit baie bronne en word nie nagegaan nie.