HD 154672 is a yellow subgiant. It is about 65 parsecs away from the Sun that is larger, but of a similar mass, as the Sun; it is, however, much older. It is very metal-rich, which is one of the reasons why it was targeted for a planet search by the N2K Consortium, which discovered the gas giant planet HD 154672 b using Doppler Spectroscopy; the discovery was reported in October 2008.
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- HD 154672 is a yellow subgiant. It is about 65 parsecs away from the Sun that is larger, but of a similar mass, as the Sun; it is, however, much older. It is very metal-rich, which is one of the reasons why it was targeted for a planet search by the N2K Consortium, which discovered the gas giant planet HD 154672 b using Doppler Spectroscopy; the discovery was reported in October 2008. The N2K collaboration chose HD 154672 primarily because it aimed to discover the correlation between a star's metallicity and the mass of orbiting planets. HD 154672 was targeted by the Magellan Telescopes. It is the host of the first planet discovered from the telescopes by N2K.
- HD 154672 — звезда, которая находится в созвездии Жертвенник на расстоянии около 215 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
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- HD 154672 — звезда, которая находится в созвездии Жертвенник на расстоянии около 215 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
- HD 154672 is a yellow subgiant. It is about 65 parsecs away from the Sun that is larger, but of a similar mass, as the Sun; it is, however, much older. It is very metal-rich, which is one of the reasons why it was targeted for a planet search by the N2K Consortium, which discovered the gas giant planet HD 154672 b using Doppler Spectroscopy; the discovery was reported in October 2008.
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