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相关论文: Specific Angular Momentum of Extrasolar Planetary …

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Recent analysis of the Doppler shift oscillations of the light from extra-solar planetary systems indicate that some of these systems have more than one large planet. In this case it has been shown that the masses of these planets can be…

天体物理学 · 物理学 2009-11-07 Michael Nauenberg

For centuries, our knowledge of planetary systems and ideas about planet formation were based on a single example, our solar system. During the last thirteen years, the discovery of ~170 planetary systems has ushered in a new era for…

天体物理学 · 物理学 2007-05-23 Eric B. Ford

The distribution of angular momentum of planets and their host stars provides important information on the formation and evolution of the planetary system. However, mysteries still remain, partly due to bias and uncertainty of the current…

地球与行星天体物理 · 物理学 2022-01-25 Jonathan H. Jiang , Remo Burn , Kristen A. Fahy , Xuan Ji , Patrick Eggenberger

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…

地球与行星天体物理 · 物理学 2021-09-22 Gregory Laughlin , Jack J. Lissauer

Extrasolar multiple-planet systems provide valuable opportunities for testing theories of planet formation and evolution. The architectures of the known multiple-planet systems demonstrate a fascinating level of diversity, which motivates…

地球与行星天体物理 · 物理学 2009-11-13 Robert A. Wittenmyer , Michael Endl , William D. Cochran , Harold F. Levison , Gregory W. Henry

Analyzing exoplanets detected by radial velocity or transit observations, we determine the multiplicity of exoplanet host stars in order to study the influence of a stellar companion on the properties of planet candidates. Matching the host…

太阳与恒星天体物理 · 物理学 2015-06-04 T. Roell , A. Seifahrt , R. Neuhäuser , M. Mugrauer

As a direct result of ongoing efforts to detect more exoplanetary systems, an ever-increasing number of multiple-planet systems are being announced. But how many of these systems are truly what they seem? In many cases, such systems are…

地球与行星天体物理 · 物理学 2013-02-22 Jonathan Horner , Robert A. Wittenmyer , Chris G. Tinney , Paul Robertson , Tobias C. Hinse , Jonathan P. Marshall

Motivated by the large number of compact extrasolar planetary systems discovered by the Kepler Mission, this paper considers perturbations due to possible additional outer planets. The discovered compact systems sometimes contain multiple…

地球与行星天体物理 · 物理学 2017-04-12 Juliette C. Becker , Fred C. Adams

Determining the orbital eccentricity of an extrasolar planet is critically important for understanding the system's dynamical environment and history. However, eccentricity is often poorly determined or entirely mischaracterized due to poor…

We investigate whether certain extra-solar multi-planet systems simultaneously follow the scaling and spacing rules of the angular-momentum-deficit model. The masses and semi-major axes of exoplanets in ten multi-planet systems are…

地球与行星天体物理 · 物理学 2020-12-18 Li-Chin Yeh , Ing-Guey Jiang , Sridhar Gajendran

The number of extrasolar planets discovered is increasing, so that more than five thousand exoplanets have been confirmed to date. Now we have an opportunity to test the validity of the laws governing planetary systems and take steps to…

地球与行星天体物理 · 物理学 2024-02-29 Mahdiyar Mousavi-Sadr

More than 100 extrasolar planets have been discovered since 1990s. Different from the solar system, these planets' orbital eccentricities cover a huge range from 0 to 0.7. Incidently, the first Kuiper Belt Object was discovered in 1992.…

天体物理学 · 物理学 2007-05-23 Ing-Guey Jiang , M. Duncan , D. N. C. Lin

The field of extrasolar planets is still, in comparison with other astrophysical topics, in its infancy. There have been about 300 or so extrasolar planets detected and their detection has been accomplished by various different techniques.…

科普物理 · 物理学 2011-06-30 Samuel J. George

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…

天体物理学 · 物理学 2008-11-26 M. A. C. Perryman

We analyzed the behavior of the rotational velocity in the parent stars of extrasolar planets. Projected rotational velocity v sin i and angular momentum were combined with stellar and planetary parameters, for a unique sample of 147 stars,…

太阳与恒星天体物理 · 物理学 2015-05-19 S. Alves , J. D. do Nascimento , J. R. De Medeiros

We analyzed the behavior of the rotational velocity in the parent stars of extrasolar planets. Projected rotational velocity v sin i and angular momentum were combined with stellar and planetary parameters, for a unique sample of 147 stars,…

太阳与恒星天体物理 · 物理学 2010-07-05 Sanzia Alves , Jose Dias do Nascimento , Jose Renan de Medeiros

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…

地球与行星天体物理 · 物理学 2009-11-24 Karan Molaverdikhani , Maryam Tabeshian

The Kepler Mission has detected dozens of compact planetary systems with more than four transiting planets. This sample provides a collection of close-packed planetary systems with relatively little spread in the inclination angles of the…

地球与行星天体物理 · 物理学 2015-12-02 Juliette C. Becker , Fred C. Adams

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…

地球与行星天体物理 · 物理学 2015-05-13 A. Eggenberger , S. Udry

We present here in full detail the evolution of the angular momentum deficit (AMD) during collisions as it was described in (Laskar, PRL,2000). Since then, the AMD has been revealed to be a key parameter for the understanding of the outcome…

地球与行星天体物理 · 物理学 2017-03-23 Jacques Laskar , Antoine Petit
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