FANDOM


OGLE-TR-132b
Extrasolar planet List of extrasolar planets
300px
Size comparison of OGLE-TR-132b with Jupiter.
Parent star

<tr> <td colspan="2">Star</td> <td>OGLE-TR-132</td></tr><tr> <td colspan="2">Constellation</td> <td>Carina</td></tr><tr> <td>Right ascension</td> <td style="text-align: center">(α)</td> <td>10h 50m 34.72s</td></tr><tr> <td>Declination</td> <td style="text-align: center">(δ)</td> <td>−61° 57′ 25.9″</td></tr><tr><td colspan="2">Distance</td><td>4892 ly
(1500 pc)</td></tr><tr><td colspan="2">Spectral type</td> <td>F</td></tr>

Orbital elements

<tr><td>Semimajor axis</td><td style="text-align: center">(a)</td> <td>0.0306 ±0.0008 AU</td></tr><tr> <td>Eccentricity</td> <td style="text-align: center">(e)</td> <td>0</td></tr><tr><td>Orbital period</td><td style="text-align: center">(P)</td> <td>1.689868 ±3e-06 d</td></tr><tr> <td>Inclination</td> <td style="text-align: center">(i)</td> <td>85 ±1°</td></tr>

Physical characteristics

<tr><td>Mass</td><td style="text-align: center">(m)</td><td>1.14 ±0.12 MJ</td></tr><tr><td>Radius</td><td style="text-align: center">(r)</td><td>1.18 ±0.07 Template:Jupiter radius</td></tr>

Discovery information

<tr> <td colspan="2">Discovery date</td> <td>14 April 2004</td></tr><tr> <td colspan="2">Discoverer(s)</td> <td>Bouchy et al.</td></tr><tr> <td colspan="2">Discovery method</td> <td>Transit</td></tr><tr> <td colspan="2">Discovery status</td> <td>Published</td></tr> <tr style="background-color: #A0B0FF;"><td align=center colspan=3>Database references</td></tr><tr valign=baseline><td colspan=2>Extrasolar Planets
Encyclopaedia
</td><td>data</td></tr><tr><td colspan=2>SIMBAD</td><td>data</td></tr>

OGLE-TR-132b is an extrasolar planet orbiting the star OGLE-TR-132.

In 2003 the Optical Gravitational Lensing Experiment (OGLE) detected periodic dimming in the star's light curve indicating a transiting, planetary-sized object. Since low-mass red dwarfs and brown dwarfs may mimic a planet radial velocity measurements were necessary to calculate the mass of the body. In 2004 the object was proved to be a new transiting extrasolar planet.[1]

File:OGLE-TR-132 b rv.pdf

The planet has a mass 1.14 times that of Jupiter. Since the planet's inclination is known, this represents the best measured true mass of the planet, rather than simply the minimum mass as is the case when the inclination is unknown. It orbits the star (OGLE-TR-132) in an extremely close orbit, even closer than the famous planets 51 Pegasi b and HD 209458 b. The planet races around the star every 1 day 16.6 hours. The radius of the planet is only 18% larger than Jupiter's, despite the heating effect by the star. Planets of its kind are sometimes called "super-hot Jupiters".[2]

See also Edit

ReferencesEdit

  1. (2004). Two new "very hot Jupiters" among the OGLE transiting candidates. Astronomy and Astrophysics 421: L13–L16.
  2. (2007). The transiting planet OGLE-TR-132b revisited with new spectroscopy and deconvolution photometry. Astronomy and Astrophysics 466 (2): 743–748.

External links Edit

Template:Commonscat-inline

Coordinates: Sky map 10h 50m 34.72s, −61° 57′ 25.9″


Ad blocker interference detected!


Wikia is a free-to-use site that makes money from advertising. We have a modified experience for viewers using ad blockers

Wikia is not accessible if you’ve made further modifications. Remove the custom ad blocker rule(s) and the page will load as expected.