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Delta Phoenicis
Star in the constellation Phoenix
Star in the constellation Phoenix
| b-v = +0.99 | u-b = +0.70
Delta Phoenicis, Latinized from δ Phoenicis, is a single, yellow-hued star in the southern constellation of Phoenix. With an apparent visual magnitude of 3.93, it is visible to the naked eye. Based upon an annual parallax shift of 22.95 mas as seen from Earth, it is located 142 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −7 km/s.
This is a G-type giant star with a stellar classification of G8.5 IIIb. It is around 2.3 billion years old with 1.47 times the mass of the Sun. The star is radiating 55 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,790 K.
References
References
- (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics.
- (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters.
- (2014). "Sloan Magnitudes for the Brightest Stars". The Journal of the American Association of Variable Star Observers.
- (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters.
- (2014). "A catalog of rotational and radial velocities for evolved stars". Astronomy & Astrophysics.
- (September 2008). "A catalogue of multiplicity among bright stellar systems". [[Monthly Notices of the Royal Astronomical Society]].
- (2007). "The abundances of nearby red clump giants". Monthly Notices of the Royal Astronomical Society.
- (2018-08-01). "Fundamental properties of red-clump stars from long-baseline H-band interferometry". [[Astronomy & Astrophysics]].
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