|
The red dot shows the location of HD 209458 in Pegasus. |
|
| Observation data Epoch J2000 Equinox J2000 |
|
|---|---|
| Constellation | Pegasus |
| Right ascension | 22h 03m 10.8s[1] |
| Declination | +18° 53′ 04″[1] |
| Apparent magnitude (V) | 7.65[1] |
| Characteristics | |
| Spectral type | G0V[1] |
| Apparent magnitude (B) | 8.24[1] |
| Apparent magnitude (K) | 6.3[1] |
| B−V color index | +0.574 ±0.014[2] |
| Variable type | EP[3] |
| Astrometry | |
| Radial velocity (Rv) | -14.8[1] km/s |
| Proper motion (μ) | RA: 28.90[1] mas/yr Dec.: -18.37[1] mas/yr |
| Parallax (π) | 21.24[1] ± 1.00[1] mas |
| Distance | 154 ly (47.1 pc) |
| Absolute magnitude (MV) | 4.28 ±0.10[2] |
| Details | |
| Mass | 1.13 -0.02+0.03[4] M☉ |
| Radius | 1.14 -0.05+0.06[4] R☉ |
| Luminosity | 1.61 L☉ |
| Temperature | 6000 ±50[2] K |
| Metallicity | 0.00 ±0.02[2] |
| Rotation | 14.4 days |
| Age | (4 ± 2) × 109[2] years |
| Other designations | |
| Database references | |
| SIMBAD | data |
| NStED | data |
| Extrasolar Planets Encyclopaedia |
data |
HD 209458 is an 8th magnitude star in the constellation Pegasus. It is very similar to our Sun, and it is classified as a yellow dwarf (spectral class G0 V). Because it is located at a distance of about 150 light years, it is not visible to the unaided eye. With good binoculars or small telescope it should be easily detectable.[1]
In 1999 two teams working independently (one team consisted of astronomers at the Geneva Observatory, the Harvard-Smithsonian Center for Astrophysics, and the Wise Observatory; the second group was the California and Carnegie Planet Search team) discovered an extrasolar planet orbiting the star by using the radial velocity planet search method. Soon after the discovery, separate teams led by David Charbonneau and Gregory W. Henry were able to detect a transit of the planet across the surface of the star making it the first known transiting extrasolar planet.[5] The planet received the designation HD 209458 b.
Because the planet transits the star, the star is dimmed by about 2% every 3.5 days making it an extrinsic variable. The variable star designation for HD 209458 is V376 Pegasi. It is the prototype of the variable class "EP" in the General Catalogue of Variable Stars, defined as stars showing eclipses by their planets.[3][6]
HD 209458 b is an extrasolar planet that orbits the Sun-like star HD 209458 in the constellation Pegasus. Spectroscopic studies first revealed the presence of a planet around HD 209458 on November 5, 1999. The planet is now under even more public scrutiny with the announcement that its atmosphere contains water vapor. Astronomers had made careful photometric measurements of several stars known to be orbited by planets, in the hope that they might observe a dip in brightness caused by the transit of the planet across the star's face. This would require the planet's orbit to be inclined such that it would pass between the Earth and the star, and previously no transits had been detected.
Travis Barman at Lowell Observatory in Flagstaff, Arizona analyzed the emission spectrum of this planet, and believes that its atmosphere contains water,[7] although previous research[8] suggests that the atmosphere is composed mostly of silicate clouds.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity |
|---|---|---|---|---|
| b | 0.69 ± 0.05 MJ | 0.045 | 3.52474541 ± 0.00000025 | 0.00 |