Summary
PA-99-N2 is a microlensing event detected in the direction of the Andromeda Galaxy in 1999.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 44m 20.89[1]s |
| Declination | +41° 28′ 44.6″[1] |
| Astrometry | |
| Distance | 2,200,000[2] ly (670,000[2] pc) |
| Database references | |
| SIMBAD | data |
| Event type | Star  |
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 44m 20.89s[1] |
| Declination | +41° 28′ 44.6″[1] |
| Epoch | J2000 |
| Distance | 2,200,000 ly (670,000 pc)[2] |
| Other designations | PA 99-N2 |
Explanations edit
One possibility for the event is that a star in the disk of M31 gravitationally lensed a red giant also in the disk. The lensing star would have a mass between 0.02 M☉ and 3.6 M☉ with the most likely value near 0.5 M☉. In this case the lens profile makes it likely[how?] that the star has a planet.[2][3]
Possible exoplanet edit
The possible exoplanet would have a mass of 6.34 Jupiter mass. If confirmed, it would be the first exoplanet found in another galaxy.[4] A similar event was seen in 1996 when a team of astronomers discovered an anomalous fluctuation in the Twin Quasar's lightcurve that seemed to be caused by a planet approximately three Earth masses in size in the quasar's lensing galaxy YGKOW G1. (However, the results remain speculative because the chance alignment that led to its discovery will never happen again; if that exoplanet could be confirmed, it would be the most distant known planet, 4 billion ly away.)[5]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b (unconfirmed) | 6.34 MJ | — | — | — | — | — |
References edit
- ^ a b c d "MEGA-ML 7". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 3 June 2018.
- ^ a b c d e "The Extrasolar Planet Encyclopaedia — PA-99-N2 b". Extrasolar Planets Encyclopaedia. 1995. Retrieved 2017-07-30.
- ^ Ingrosso, G.; Paolis, F. DE; Novati, S. Calchi; Jetzer, PH.; Nucita, A. A.; Zakharov, A. F. (2012). "Detection of Exoplanets in M31 with Pixel-Lensing: The Event Pa-99-N2 Case". The Twelfth Marcel Grossmann Meeting. The Twelfth Marcel Grossmann Meeting: On Recent Developments in Theoretical and Experimental General Relativity. p. 2191. arXiv:1001.2105. Bibcode:2012mgm..conf.2191I. doi:10.1142/9789814374552_0433. ISBN 978-981-4374-51-4.
- ^ An, Jin H.; Evans, N. W.; Kerins, E.; Baillon, P.; Calchi Novati, S.; Carr, B. J.; Creze, M.; Giraud‐Heraud, Y.; Gould, A.; Hewett, P.; Jetzer, Ph.; Kaplan, J.; Paulin‐Henriksson, S.; Smartt, S. J.; Tsapras, Y.; Valls‐Gabaud, D. (February 2004). "The Anomaly in the Candidate Microlensing Event PA‐99‐N2". The Astrophysical Journal. 601 (2): 845–857. arXiv:astro-ph/0310457. Bibcode:2004ApJ...601..845A. doi:10.1086/380820. S2CID 8312033.
- ^ Govert Schilling (6 July 1996). "Do alien worlds throng faraway galaxy?". New Scientist. No. 2037.