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Binary-binary interactions are important in a number of astrophysical contexts including dense stellar systems such as globular clusters. Although less frequent than binary-single encounters, binary-binary interactions lead to a much richer…

High Energy Astrophysical Phenomena · Physics 2020-03-18 Adrian S. Hamers , Johan Samsing

Binary systems are very common among field stars. While this relatively small number of planets in binaries is probably partly due to strong observational biases, there is, however, statistical evidence that planets are indeed less frequent…

Earth and Planetary Astrophysics · Physics 2020-02-28 Francesco Marzari , Philippe Thebault

Asteroid binaries found amongst the Near-Earth objects are believed to have formed from rotational fission. In this paper, we aim to study the dynamical evolution of asteroid systems the moment after fission. The initial condition is…

Earth and Planetary Astrophysics · Physics 2022-09-14 Alex Ho , Margrethe Wold , Mohammad Poursina , John T. Conway

The statistical properties of planets in binaries were investigated. Any difference to planets orbiting single stars can shed light on the formation and evolution of planetary systems. As planets were found around components of binaries…

Astrophysics · Physics 2009-11-11 S. Desidera , M. Barbieri

In the past decade, the number of known binary near-Earth asteroids has more than quadrupled and the number of known large main belt asteroids with satellites has doubled. Half a dozen triple asteroids have been discovered, and the…

Earth and Planetary Astrophysics · Physics 2016-08-31 Jean-Luc Margot , Petr Pravec , Patrick Taylor , Benoît Carry , Seth Jacobson

A binary star system is the most common result of the star formation process, and binary companions can disrupt both the formation of terrestrial planets and their long term prospects for stability. We present results from a large set of…

Astrophysics · Physics 2007-05-24 Elisa V. Quintana , Jack J. Lissauer

We calculate herein the late stages of terrestrial planet accumulation around a solar type star that has a binary companion with semimajor axis larger than the terrestrial planet region. We perform more than one hundred simulations to…

Astrophysics · Physics 2011-02-11 Elisa V. Quintana , Fred C. Adams , Jack J. Lissauer , John E. Chambers

The present dynamical configuration of planets in binary star systems may not reflect their formation process since the binary orbit may have changed in the past after the planet formation process was completed. An observed binary system…

Astrophysics · Physics 2009-11-13 F. Marzari , M. Barbieri

Spurred by the discovery of numerous exoplanets in multiple systems, binaries have become in recent years one of the main topics in planet formation research. Numerous studies have investigated to what extent the presence of a stellar…

Earth and Planetary Astrophysics · Physics 2017-11-29 Ph. Thebault , N. Haghighipour

In this work, we investigate the dynamical effects of a sequence of close encounters over 200 Myr varying in the interval of 10000 -- 100000 au between a binary star system and passing stars with masses ranging from 0.1$M_{\odot}$ to…

Earth and Planetary Astrophysics · Physics 2023-06-14 David Bancelin , Thomas Nordlander , Elke Pilat-Lohinger , Birgit Loibnegger

The planet formation process and subsequent planet migration may lead to configurations resulting in strong dynamical interactions among the various planets. Well-studied possible outcomes include collisions between planets, scattering…

Earth and Planetary Astrophysics · Physics 2010-07-09 Philipp Podsiadlowski , Saul Rappaport , John M. Fregeau , Rosemary A. Mardling

Strong encounters between single stars and binaries play a pivotal role in the evolution of star clusters. Such encounters can also dramatically modify the orbital parameters of binaries, exchange partners in and out of binaries, and are a…

Solar and Stellar Astrophysics · Physics 2015-08-06 Aaron M. Geller , Nathan W. C. Leigh

Understanding the origin of planets that have formed in binary stars is fundamental to constrain theories of binary and planet formation. The planet occurrence rate in binaries with a separation $\lesssim 50$ AU is only $\sim$ one third…

Earth and Planetary Astrophysics · Physics 2018-12-19 Giacomo Fragione

Although it is commonly agreed that the presence of a close stellar companion is likely to affect planet formation and evolution, the precise effects and their actual impact on planet occurrence and properties are still debated. In…

Astrophysics · Physics 2019-08-19 A. Eggenberger , S. Udry

We explore the impact of outer stellar companions on the occurrence rate of giant planets detected with radial velocities. We searched for stellar and planetary companions to a volume-limited sample of solar-type stars within 25 pc. Using…

The locations of the fully despun, double synchronous end states of tidal evolution are derived for spherical components. With the exception of nearly equal-mass binaries, binary asteroid systems are in the midst of lengthy tidal…

Earth and Planetary Astrophysics · Physics 2015-03-18 Patrick A. Taylor , Jean-Luc Margot

We investigate the orbital dynamics of circumbinary planetary systems with two planets around a circular or eccentric orbit binary. The orbits of the two planet are initially circular and coplanar to each other, but misaligned with respect…

Earth and Planetary Astrophysics · Physics 2021-12-15 Cheng Chen , Stephen H. Lubow , Rebecca G. Martin

Stellar perturbations affect planet-formation in binary systems. Recent studies show that the planet-formation stage of mutual accretion of km-sized planetesimals is most sensitive to binary effects. In this paper, the condition for…

Earth and Planetary Astrophysics · Physics 2015-05-18 Ji-Wei Xie , Ji-Lin Zhou , Jian Ge

Roughly half of Solar-type planet hosts have stellar companions, so understanding how these binary companions affect the formation and evolution of planets is an important component to understanding planetary systems overall. Measuring the…

Disk material has been observed around both components of some young close binary star systems. It has been shown that if planets form at the right places within such disks, they can remain dynamically stable for very long times. Herein, we…

Astrophysics · Physics 2009-11-11 Elisa V. Quintana , Jack J. Lissauer
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