A Transiting Planet of a Sun-like Star
| dc.creator | McCullough, P. R. | |
| dc.creator | Stys, J. E. | |
| dc.creator | Valenti, Jeff A. | |
| dc.creator | Johns-Krull, C. M. | |
| dc.creator | Janes, K. A. | |
| dc.creator | Heasley, J. N. | |
| dc.creator | Bye, B. A. | |
| dc.creator | Dodd, C. | |
| dc.creator | Fleming, S. W. | |
| dc.creator | Pinnick, A. | |
| dc.creator | Bissinger, R. | |
| dc.creator | Gary, B. L. | |
| dc.creator | Howell, P. J. | |
| dc.creator | Vanmunster, T. | |
| dc.date | 2006-05-17 | |
| dc.date.accessioned | 2026-07-07T10:39:01Z | |
| dc.date.available | 2026-07-07T10:39:01Z | |
| dc.description | A planet transits an 11th magnitude, G1V star in the constellation Corona Borealis. We designate the planet XO-1b, and the star, XO-1, also known as GSC 02041-01657. XO-1 lacks a trigonometric distance; we estimate it to be 200+-20 pc. Of the ten stars currently known to host extrasolar transiting planets, the star XO-1 is the most similar to the Sun in its physical characteristics: its radius is 1.0+-0.08 R_Sun, its mass is 1.0+-0.03 M_Sun, V sini < 3 km/s, and its metallicity [Fe/H] is 0.015+-0.04. The orbital period of the planet XO-1b is 3.941534+-0.000027 days, one of the longer ones known. The planetary mass is 0.90+-0.07 M_Jupiter, which is marginally larger than that of other transiting planets with periods between 3 and 4 days. Both the planetary radius and the inclination are functions of the spectroscopically determined stellar radius. If the stellar radius is 1.0+-0.08 R_Sun, then the planetary radius is 1.30+-0.11 R_Jupiter and the inclination of the orbit is 87.7+-1.2 degrees. We have demonstrated a productive international collaboration between professional and amateur astronomers that was important to distinguishing this planet from many other similar candidates. | |
| dc.description | 31 pages, 9 figures, accepted for part 1 of ApJ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0605414 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0605414 | |
| dc.identifier | Astrophys.J.648:1228-1238,2006 | |
| dc.identifier | doi:10.1086/505651 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/180887 | |
| dc.subject | Astrophysics | |
| dc.title | A Transiting Planet of a Sun-like Star | |
| dc.type | text |