HD 47536
|
Stern HD 47536 |
|||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| AladinLite | |||||||||||||
|
Observation dates equinox : J2000.0 , epoch : J2000.0 |
|||||||||||||
| Constellation | Big dog | ||||||||||||
| Right ascension | 06 h 37 m 47.62 s | ||||||||||||
| declination | -32 ° 20 ′ 23.1 ″ | ||||||||||||
| Apparent brightness | 5.25 likes | ||||||||||||
| Typing | |||||||||||||
| B − V color index | +1.18 | ||||||||||||
| U − B color index | +1.12 | ||||||||||||
| Spectral class | K1 III | ||||||||||||
| Astrometry | |||||||||||||
| Radial velocity | (+78.8 ± 0.8) km / s | ||||||||||||
| parallax | (8.11 ± 0.23) mas | ||||||||||||
| distance | (402 ± 11) ly (123 ± 3) pc |
||||||||||||
| Visual absolute brightness M vis | −0.2 mag | ||||||||||||
| Proper movement | |||||||||||||
| Rec. Share: | (+108.06 ± 0.20) mas / a | ||||||||||||
| Dec. portion: | (+64.60 ± 0.24) mas / a | ||||||||||||
| Physical Properties | |||||||||||||
| radius | (23 ± 2) R ☉ | ||||||||||||
| Luminosity |
180 L ☉ |
||||||||||||
| Effective temperature | 4380 K | ||||||||||||
| Metallicity [Fe / H] | −0.68 | ||||||||||||
| Age | approx. 9 bill. a | ||||||||||||
|
Other names and catalog entries |
|||||||||||||
|
|||||||||||||
| annotation | |||||||||||||
|
|||||||||||||
HD 47536 is a 400 light-years distant giant of the spectral class K1 with an apparent magnitude of 5.3 mag. The star is orbited by at least one substellar object, the confirmation of a second is still pending.
companion
In 2003 Setiawan et al. With the help of the radial velocity method a companion around HD 47536, for which they determined an orbital period of 712 days and a minimum mass of less than 10 Jupiter's masses, which makes the object with the systematic name HD 47536 b a potential exoplanet .
In the course of subsequent observations of the star with Coralie and FEROS, Setiawan et al. Notes on another spectroscopic companion. HD 47536 c has a longer orbital period of about 2500 days and has a minimum mass of about 7 Jupiter's masses. Based on this discovery, they also determined a revised solution for the inner companion with an orbital period of around 430 days and a minimum mass of around 5 Jupiter's masses. The confirmation of the external companion is currently pending (as of the end of 2010).
Web links
Individual evidence
- ↑ a b c Hipparcos catalog (ESA 1997)
- ↑ a b Bright Star Catalog
- ↑ Pulkovo radial velocities for 35493 HIP stars
- ↑ a b c Hipparcos, the New Reduction (van Leeuwen, 2007)