OGLE-2006-BLG-109L
 Location of OGLE-2006-BLG-109L (green) in the constellation of Scorpius. | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Scorpius |
| Right ascension | 17h 52m 35.0s[1] |
| Declination | –30° 05′ 16″[1] |
| Apparent magnitude (V) | 17.17 |
| Characteristics | |
| Spectral type | Unsure (probably M0V) |
| Astrometry | |
| Distance | 4,920 ± 390 ly (1,510 ± 120 pc) |
| Details | |
| Mass | 0.51 ± 0.04 M☉ |
| Temperature | ~4,000 K |
| Other designations | |
EWS 2006-BUL-109 | |
| Database references | |
| SIMBAD | data |
OGLE-2006-BLG-109L (where the last 'L' stands for lens) is a dim magnitude 17 M0V galactic bulge star approximately 4,920 light-years away in the constellation of Scorpius.[1]
Planetary system
[edit]In 2008, two extrasolar planets were discovered around the star using gravitational microlensing. The two planets are at a distance from their star that make them suspected analogs of Jupiter and Saturn.[2]
The star is surrounded by a planetary system consisting of at least two planets: b with a mass of 0.727 of Jupiter and c with the mass of approximately 0.271 of Jupiter. Their mass ratios, distance ratios, and equilibrium temperatures are similar to those of Jupiter and Saturn in the Solar System as well as the 47 UMa system.[2]
Both planets were discovered simultaneously by gravitational microlensing in a common effort by the Optical Gravitational Lensing Experiment, microFUN, MOA, PLANET and RoboNet collaborations, as announced on 14 February 2008. This is the first planetary system where more than one planet was detected using gravitational microlensing.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 0.727 ± 0.06 MJ | 2.3 ± 0.5 | 1790 ± 548 | ? | — | — |
| c | 0.271 ± 0.022 MJ | 4.5 ± 1 | 4931 ± 1750 | 0.15 ± 0.1 | — | — |
See also
[edit]References
[edit]- ^ a b c "NAME OGLE 2006-BLG-109". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2009-04-30.
- ^ a b Gaudi, B. S.; et al. (2008). "Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing". Science. 319 (5865): 927–930. arXiv:0802.1920. Bibcode:2008Sci...319..927G. doi:10.1126/science.1151947. PMID 18276883. S2CID 119281787.
External links
[edit]- Britt, Robert Roy (2008-02-14). "Solar System Like Ours Found". Space.com. Retrieved 2008-06-27.
- "Discovery of a Jupiter/Saturn Analog in OGLE-2006-BLG-109". MicroFUN. Retrieved 2008-06-27.
- Dominik, Martin (2006-02-11). "The unlonely planets — Discovery of a Jupiter/Saturn analogue". ARTEMiS. Archived from the original on 2012-02-10. Retrieved 2008-06-27.
- Overbye, Dennis (2008-02-14). "Scientists Find Solar System Like Ours". The New York Times. Retrieved 2008-06-27.
- Rincon, Paul (2008-04-06). "Solar System's 'look-alike' found". BBC News. Retrieved 2008-06-27.
- "OGLE-06-109L". Exoplanets. Archived from the original on 2016-03-03. Retrieved 2009-04-30.
