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Open AccessJournal ArticleDOI

Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

B. S. Gaudi, +70 more
- 15 Feb 2008 - 
- Vol. 319, Iss: 5865, pp 927-930
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TLDR
Two planets with masses that could not have been detected with other techniques are identified; their discovery from only six confirmed microlensing planet detections suggests that solar system analogs may be common.
Abstract
Searches for extrasolar planets have uncovered an astonishing diversity of planetary systems, yet the frequency of solar system analogs remains unknown. The gravitational microlensing planet search method is potentially sensitive to multiple-planet systems containing analogs of all the solar system planets except Mercury. We report the detection of a multiple-planet system with microlensing. We identify two planets with masses of ∼0.71 and ∼0.27 times the mass of Jupiter and orbital separations of ∼2.3 and ∼4.6 astronomical units orbiting a primary star of mass ∼0.50 solar mass at a distance of ∼1.5 kiloparsecs. This system resembles a scaled version of our solar system in that the mass ratio, separation ratio, and equilibrium temperatures of the planets are similar to those of Jupiter and Saturn. These planets could not have been detected with other techniques; their discovery from only six confirmed microlensing planet detections suggests that solar system analogs may be common.

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Journal ArticleDOI

The Occurrence and Architecture of Exoplanetary Systems

TL;DR: A review of the current knowledge of the occurrence of planets around other stars, their orbital distances and eccentricities, the orbital spacings and mutual inclinations in multi-planet systems, the orientation of the host star's rotation axis, and the properties of planets in binary-star systems can be found in this paper.
Journal ArticleDOI

The HARPS search for southern extra-solar planets - XXXI. The M-dwarf sample

TL;DR: In this paper, the authors used a fraction of the guaranteed time on the ESO/HARPS spectrograph to estimate the radial velocities of 102 southern nearby M dwarfs, and then applied systematic searches for long-term trends, periodic signals, and Keplerian orbits.
Journal ArticleDOI

One or more bound planets per Milky Way star from microlensing observations

Arnaud Cassan, +70 more
- 12 Jan 2012 - 
TL;DR: It is concluded that stars are orbited by planets as a rule, rather than the exception, and that of stars host Jupiter-mass planets 0.5–10 au (Sun–Earth distance) from their stars.
Book

The Exoplanet Handbook

TL;DR: In this paper, the authors present an overview of the solar system and its evolution, including the formation and evolution of stars, asteroids, and free-floating planets, as well as their internal and external structures.
References
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Journal ArticleDOI

A Jupiter-Mass Companion to a Solar-Type Star

Michel Mayor, +1 more
- 23 Nov 1995 - 
TL;DR: The presence of a Jupiter-mass companion to the star 51 Pegasi is inferred from observations of periodic variations in the star's radial velocity as discussed by the authors, which would be well inside the orbit of Mercury in our Solar System.
Journal ArticleDOI

The Planet-Metallicity Correlation

TL;DR: In this paper, the authors identify a subset of 850 stars that have Doppler observations sufficient to detect uniformly all planets with radial velocity semiamplitudes K > 30 m s-1 and orbital periods shorter than 4 yr, and determine that fewer than 3% of stars with -0.5 + 0.3 dex, 25% of observed stars have detected gas giant planets.
Journal ArticleDOI

A planetary system around the millisecond pulsar PSR1257 + 12

TL;DR: In this article, the authors used the 305m Arecibo radiotelescope to make precise timing measurements of pulses from the recently discovered 6.2-ms pulsar PSR1257 +12 (ref. 2).
Journal ArticleDOI

Orbital migration of the planetary companion of 51 Pegasi to its present location

TL;DR: In this paper, the authors show that if the companion is indeed a gas-giant planet, it is extremely unlikely to have formed at its present location, and suggest instead that the planet probably formed by gradual accretion of solids and capture of gas at a much larger distance from the star (∼5 AU), and that it subsequently migrated inwards through interactions with the remnants of the circumstellar disk.
Journal ArticleDOI

Catalog of nearby exoplanets

TL;DR: In this article, the authors present a catalog of nearby exoplanets, which contains the 172 known low-mass companions with orbits established through radial velocity and transit measurements around stars within 200 pc, including five previously unpublished ex-oplanets orbiting the stars HD 11964, HD 66428, HD 99109, HD 107148 and HD 164922.
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