Clever Geek Handbook
📜 ⬆️ ⬇️

HD 208527

HD 208527 is a star located in the constellation Pegasus at a distance of about 1044 light years from Earth . At least one planet orbits a star.

HD 208527
Star
Observational data
( Age J2000.0 )
Type ofSingle star
Right ascension
Declination
Distance1044 St. years (320.2 pc ) [1]
Visible magnitude ( V )6.4 [1]
ConstellationPegasus
Astrometry
Radial velocity ( R v )4.79 [2] km / s
Own movement (μ)RA: 2.00 [2]
Dec: 15.30 [2]
Parallax (π)2.48 ± 0.38 [2] mas
Absolute magnitude (V)–1.24 [1]
Characteristics
Spectral classM1III [1]
Color Index ( B - V )1.70 ± 0.02 [1]
physical characteristics
Weight1.6 ± 0.4 [1] M ☉
Radius51.1 ± 8.3 [1] R ☉
Age2.0 ± 1.3 billion [1] years
Temperature4035 ± 65 [1] K
Metallicity[Fe / H] = - 0.09 ± 0.16 [1]
Rotation3.6 km / s -1 [1]
Other designations
BD +20 5046 , FK5 1579 , HD 208527 , HIC 108296 , HIP 108296 , HR 8372 , IRC +20524 , PPM 113798 , SAO 90112 , 2MASS J21562398 + 2114233, AG +21 2431, GC 30710, GCRV 13785, GJ 841.1, GSC 01691-01788, N30 4835, PLX 5301.02, PMC 90-93 1119, SKY # 41804, SRS 31579, TYC 1691-1788-1, uvby98 100208527, YZ 21 8460, Zkh 323
Database Information
SIMBADdata
Sources: [2]

Content

Features

HD 208527 - a star of 6.4 visible magnitude; for the first time in astronomical literature is mentioned in the catalog of Henry Draper , published at the beginning of the XX century . It was previously believed that the star is an orange dwarf, but recent studies have shown that it is a large red giant . [1] The mass of the star is equal to 1.6 the mass of the Sun and in size it exceeds our daylight by 51 times. The surface temperature of HD 208527 is approximately 4035 Kelvin . Her age is estimated at approximately two billion years.

Planet System

In 2012, a group of South Korean astronomers from the Bohyunsan Optical Astronomy Observatory announced the discovery [1] of the planet HD 208527 b in the system. This is a gas giant , surpassing Jupiter in mass by 9.9 times. The planet is drawn at a distance of 2.1 AU from the parent star, making a complete revolution of 875 days. The discovery of the planet was made by Doppler spectroscopy .

Planet
Weight
( M J )
Radius
( R J )
Circulation period
( days )
Semimajor axis
orbits ( a.u. )
Eccentricity
orbits
b9.9 ± 1.7-875.5 ± 5.82.1 ± 0.20.08 ± 0.04

Notes

  1. ↑ 1 2 3 4 5 6 7 8 9 10 11 12 13 B.-C. Lee, I. Han, M.-G. Park. Planetary companions orbiting M giants HD 208527 and HD 220074 (English) . Arxiv.org (Nov 9, 2012). Date of treatment March 2, 2013.
  2. ↑ 1 2 3 4 5 SIMBAD - HD 208527 in the SIMBAD database . Date of treatment March 2, 2013.
  3. ↑ 1 2 3 4 Gaia Data Release 2 - 2018.
    <a href=" https://wikidata.org/wiki/Track:Q51905050 "> </a>

See also

  • Pegasus constellation star list

Links

  • HD 208527 in the Encyclopedia of Extrasolar Planets
  • HD 208527 Online Planetary Systems
Source - https://ru.wikipedia.org/w/index.php?title=HD_208527&oldid=53506728


More articles:

  • Demidovo (Gus-Khrustalny district)
  • Evstafiev, Nikolai Alexandrovich
  • Evstigneev, Alexander Dmitrievich
  • Red Cordon (Zarenda district)
  • Oakwood Cemetery (Austin)
  • Ibn Hibban
  • List of Heads of State in 406
  • Azam, Aegid Quirin
  • Intercession Church (Irkutsk)
  • Alexis, Jacques-Stephen

All articles

Clever Geek | 2019