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Related papers: Extrasolar Planets in the Classroom

200 papers

The discovery of the first extra-solar planet surrounding a main-sequence star was announced in 1995, based on very precise radial velocity (Doppler) measurements. A total of 34 such planets were known by the end of March 2000, and their…

Astrophysics · Physics 2008-11-26 M. A. C. Perryman

The detection of thousands of extrasolar planets by the transit method naturally raises the question of whether potential extrasolar observers could detect the transits of the Solar System planets. We present a comprehensive analysis of the…

Earth and Planetary Astrophysics · Physics 2017-09-08 R. Wells , K. Poppenhaeger , C. A. Watson , R. Heller

Exoplanets, or planets outside our own solar system, have long been of interest to astronomers; however, only in the past two decades have scientists had the technology to characterize and study planets so far away from us. With advanced…

Earth and Planetary Astrophysics · Physics 2018-05-09 Jason Wei

I present a review of observational efforts to study known extrasolar planets by methods that are complementary to the radial velocity technique. I describe the current state of attempts to detect and characterize such planets by…

Astrophysics · Physics 2007-05-23 David Charbonneau

Observational surveys for extrasolar planets probe the diverse outcomes of planet formation and evolution. These surveys measure the frequency of planets with different masses, sizes, orbital characteristics, and host star properties. Small…

Earth and Planetary Astrophysics · Physics 2013-05-03 Andrew W. Howard

The primary difficulty with using transits to discover extrasolar planets is the low probability a planet has of transiting its parent star. One way of overcoming this difficulty is to search for transits in dense stellar fields, such as…

Astrophysics · Physics 2009-10-31 B. Scott Gaudi

I present a review of astrometric techniques and instrumentation utilized to search for, detect, and characterize extra-solar planets. First, I briefly summarize the properties of the present-day sample of extrasolar planets, in connection…

Astrophysics · Physics 2009-11-11 A. Sozzetti

Thousands of extrasolar planets have been discovered, and it is clear that the galactic planetary census draws on a diversity greatly exceeding that exhibited by the solar system's planets. We review significant landmarks in the chronology…

Earth and Planetary Astrophysics · Physics 2021-09-22 Gregory Laughlin , Jack J. Lissauer

The discovery of transiting extrasolar planets has enabled us a number of interesting stduies. Transit photometry reveals the radius and the orbital inclination of transiting planets, and thereby we can learn the true mass and the density…

Earth and Planetary Astrophysics · Physics 2015-05-13 Norio Narita

Of the over 200 known extrasolar planets, 14 exhibit transits in front of their parent stars as seen from Earth. Spectroscopic observations of the transiting planets can probe the physical conditions of their atmospheres. One such technique…

Astrophysics · Physics 2009-10-16 L. Jeremy Richardson , Drake Deming , Karen Horning , Sara Seager , Joseph Harrington

Many of the planets discovered via the radial velocity technique are hot Jupiters in 3-5 day orbits with ~10$% chance of transiting their parent star. However, radial velocity surveys for extra-solar planets generally require substantial…

Astrophysics · Physics 2007-05-23 Stephen R. Kane , Jian Ge

We investigate a new approach to the detection of companions to extrasolar planets beyond the transit method. We discuss the possibility of the existence of binary planets. We develop a method based on the imaging of a planet-companion as…

Astrophysics · Physics 2007-05-23 J. Cabrera , J. Schneider

We propose that the presence of additional planets in extrasolar planetary systems can be detected by long-term transit timing studies. If a transiting planet is on an eccentric orbit then the presence of another planet causes a secular…

Astrophysics · Physics 2008-11-26 Jeremy S. Heyl , Brett J. Gladman

Over 300 extrasolar planets have been found since 1992, showing that planetary systems are common and exhibit an outstanding variety of characteristics. As the number of detections grows and as models of planet formation progress to account…

Earth and Planetary Astrophysics · Physics 2015-05-13 A. Eggenberger , S. Udry

Transiting planet systems offer an unique opportunity to observationally constrain proposed models of the interiors (radius, composition) and atmospheres (chemistry, dynamics) of extrasolar planets. The spectacular successes of ground-based…

Earth and Planetary Astrophysics · Physics 2009-12-07 A. Sozzetti , C. Afonso , R. Alonso , D. L. Blank , C. Catala , H. Deeg , J. L. Grenfell , C. Hellier , D. W. Latham , D. Minniti , F. Pont , H. Rauer

The search for extrasolar Earth-like planets is underway. Over 100 extrasolar giant planets are known to orbit nearby sun-like stars, including several in multiple-planet systems. These planetary systems are stepping stones for the search…

Astrophysics · Physics 2009-11-07 S. Seager

Future surveys for transiting extrasolar planets, including the space-based mission Kepler (Borucki et al 2003), are expected to detect hundreds of Jovian mass planets and tens of terrestrial mass planets. For many of these newly discovered…

Astrophysics · Physics 2011-09-01 Matthew J. Holman , Norman W. Murray

The growing rate of increase in the number of the discovered extra-solar planets which has consequently raised the enthusiasm to explore the universe in hope of finding earth-like planets has resulted in the wide use of Gravitational…

Earth and Planetary Astrophysics · Physics 2009-11-24 Karan Molaverdikhani , Maryam Tabeshian

Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmospheres and surfaces with spectroscopy. Rocky planets within…

Earth and Planetary Astrophysics · Physics 2009-11-17 J. Kasting , W. Traub , A. Roberge , A. Leger , A. Schwartz , A. Wooten , A. Vosteen , A. Lo , A. Brack , A. Tanner , A. Coustenis , B. Lane , B. Oppenheimer , B. Mennesson , B. Lopez , C. Grillmair , C. Beichman , C. Cockell , C. Hanot , C. McCarthy , C. Stark , C. Marois , C. Aime , D. Angerhausen , D. Montes , D. Wilner , D. Defrere , D. Mourard , D. Lin , E. Kite , E. Chassefiere , F. Malbet , F. Tian , F. Westall , G. Illingworth , G. Vasisht , G. Serabyn , G. Marcy , G. Bryden , G. White , G. Laughlin , G. Torres , H. Hammel , H. Ferguson , H. Shibai , H. Rottgering , J. Surdej , J. Wiseman , J. Ge , J. Bally , J. Krist , J. Monnier , J. Trauger , J. Horner , J. Catanzarite , J. Harrington , J. Nishikawa , K. Stapelfeldt , K. von Braun , K. Biazzo , K. Carpenter , K. Balasubramanian , L. Kaltenegger , M. Postman , M. Spaans , M. Turnbull , M. Levine , M. Burchell , M. Ealey , M. Kuchner , M. Marley , M. Dominik , M. Mountain , M. Kenworthy , M. Muterspaugh , M. Shao , M. Zhao , M. Tamura , N. Kasdin , N. Haghighipour , N. Kiang , N. Elias , N. Woolf , N. Mason , O. Absil , O. Guyon , O. Lay , P. Borde , P. Fouque , P. Kalas , P. Lowrance , P. Plavchan , P. Hinz , P. Kervella , P. Chen , R. Akeson , R. Soummer , R. Waters , R. Barry , R. Kendrick , R. Brown , R. Vanderbei , R. Woodruff , R. Danner , R. Allen , R. Polidan , S. Seager , S. MacPhee , S. Hosseini , S. Metchev , S. Kafka , S. Ridgway , S. Rinehart , S. Unwin , S. Shaklan , T. ten Brummelaar , T. Mazeh , V. Meadows , W. Weiss , W. Danchi , W. Ip , Y. Rabbia

In our solar system massive outer planets dominate in terms of both mass and angular momentum, but few such planets are among the more than 4000 currently confirmed exoplanets, and none of these have accurately determined densities. Here I…

Earth and Planetary Astrophysics · Physics 2020-02-14 Derek Buzasi
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