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We consider the possibility of detecting and tracking the hypothesized Planet 9 or other unknown planetary-mass distant solar system members, generically called Planet X, with a combination of CMB and optical imaging surveys. Planets are…

Earth and Planetary Astrophysics · Physics 2018-12-21 Eric J. Baxter , Bhuvnesh Jain , Cullen Blake , Gary Bernstein , Mark Devlin , Gil Holder

The Solar system beyond Neptune is believed to house a population of small primordial bodies left over from the planet formation process. The region up to heliocentric distance $\sim 50 AU$ (a.k.a. the Kuiper Belt) may be the source of the…

Astrophysics · Physics 2009-10-28 Renu Malhotra

For centuries, astronomers have discussed the possibility of inhabited worlds - from Herschel's 18th-century observations suggesting Mars may host life, to the systematic search for technosignatures that began in the 1960s using radio…

Instrumentation and Methods for Astrophysics · Physics 2025-10-22 Beatriz Villarroel , Wesley A. Watters , Alina Streblyanska , Enrique Solano , Stefan Geier , Lars Mattsson

Asymmetric debris discs have been found around stars other than the Sun; asymmetries are sometimes attributed to perturbations induced by unseen planets. The presence or absence of asymmetries in our own trans-Neptunian belt remains…

Earth and Planetary Astrophysics · Physics 2022-03-01 C. de la Fuente Marcos , R. de la Fuente Marcos

Over the past several decades, thousands of planets have been discovered outside of our Solar System. These planets exhibit enormous diversity, and their large numbers provide a statistical opportunity to place our Solar System within the…

Thousands of exoplanets have been found with many widely different from the ones in our own system. Despite the success, systems with planets in wide orbits analogous to those of Jupiter and Saturn, in the critical first several hundred…

The gap between two component debris disks is often taken to be carved by intervening planets scattering away the remnant planetesimals. We employ N-body simulations to determine how the time needed to clear the gap depends on the location…

Earth and Planetary Astrophysics · Physics 2016-09-02 Andrew Shannon , Amy Bonsor , Quentin Kral , Elisabeth Matthews

Our understanding of the Solar System has been revolutionized over the past decade by the finding that the orbits of the planets are inherently chaotic. In extreme cases, chaotic motions can change the relative positions of the planets…

Astrophysics · Physics 2007-05-23 N. Murray , M. Holman

Are there other planetary systems in our Universe? Indirect evidence has been found for planets orbiting other stars in our galaxy: the gravity of orbiting planets makes the star wobble, and the resulting periodic Doppler shifts have been…

Astrophysics · Physics 2007-05-23 Edward A. Baltz , Paolo Gondolo

New data on the distribution of distant trans-Neptunian objects and on the properties of comets indicate the importance of dynamical processes in the outer part of the protoplanetary disk in the formation of the observed structure of the…

Earth and Planetary Astrophysics · Physics 2020-04-08 V. V. Emel'yanenko

Planets with radii between that of the Earth and Neptune (hereafter referred to as sub-Neptunes) are found in close-in orbits around more than half of all Sun-like stars. Yet, their composition, formation, and evolution remain poorly…

Earth and Planetary Astrophysics · Physics 2023-11-30 R. Luque , H. P. Osborn , A. Leleu , E. Pallé , A. Bonfanti , O. Barragán , T. G. Wilson , C. Broeg , A. Collier Cameron , M. Lendl , P. F. L. Maxted , Y. Alibert , D. Gandolfi , J. -B. Delisle , M. J. Hooton , J. A. Egger , G. Nowak , M. Lafarga , D. Rapetti , J. D. Twicken , J. C. Morales , I. Carleo , J. Orell-Miquel , V. Adibekyan , R. Alonso , A. Alqasim , P. J. Amado , D. R. Anderson , G. Anglada-Escudé , T. Bandy , T. Bárczy , D. Barrado Navascues , S. C. C. Barros , W. Baumjohann , D. Bayliss , J. L. Bean , M. Beck , T. Beck , W. Benz , N. Billot , X. Bonfils , L. Borsato , A. W. Boyle , A. Brandeker , E. M. Bryant , J. Cabrera , S. Carrazco Gaxiola , D. Charbonneau , S. Charnoz , D. R. Ciardi , W. D. Cochran , K. A. Collins , I. J. M. Crossfield , Sz. Csizmadia , P. E. Cubillos , F. Dai , M. B. Davies , H. J. Deeg , M. Deleuil , A. Deline , L. Delrez , O. D. S. Demangeon , B. -O. Demory , D. Ehrenreich , A. Erikson , E. Esparza-Borges , B. Falk , A. Fortier , L. Fossati , M. Fridlund , A. Fukui , J. Garcia-Mejia , S. Gill , M. Gillon , E. Goffo , Y. Gomez Maqueo Chew , M. Güdel , E. W. Guenther , M. N. Günther , A. P. Hatzes , Ch. Helling , K. M. Hesse , S. B. Howell , S. Hoyer , K. Ikuta , K. G. Isaak , J. M. Jenkins , T. Kagetani , L. L. Kiss , T. Kodama , J. Korth , K. W. F. Lam , J. Laskar , D. W. Latham , A. Lecavelier des Etangs , J. P. D. Leon , J. H. Livingston , D. Magrin , R. A. Matson , E. C. Matthews , C. Mordasini , M. Mori , M. Moyano , M. Munari , F. Murgas , N. Narita , V. Nascimbeni , G. Olofsson , H. L. M. Osborne , R. Ottensamer , I. Pagano , H. Parviainen , G. Peter , G. Piotto , D. Pollacco , D. Queloz , S. N. Quinn , A. Quirrenbach , R. Ragazzoni , N. Rando , F. Ratti , H. Rauer , S. Redfield , I. Ribas , G. R. Ricker , A. Rudat , L. Sabin , S. Salmon , N. C. Santos , G. Scandariato , N. Schanche , J. E. Schlieder , S. Seager , D. Ségransan , A. Shporer , A. E. Simon , A. M. S. Smith , S. G. Sousa , M. Stalport , Gy. M. Szabó , N. Thomas , A. Tuson , S. Udry , A. M. Vanderburg , V. Van Eylen , V. Van Grootel , J. Venturini , I. Walter , N. A. Walton , N. Watanabe , J. N. Winn , T. Zingales

Several stars show deep transits consistent with discs of roughly 1 Solar radius seen at moderate inclinations, likely surrounding planets on eccentric orbits. We show that this configuration arises naturally as a result of planet-planet…

Earth and Planetary Astrophysics · Physics 2024-05-16 Alexander J. Mustill , Melvyn B. Davies , Matthew A. Kenworthy

Over the last few years, several close orbiting ($\sim 0.05$ AU) large mass planets ($M \sim M_{Jupiter}$) of nearby stars have been discovered. Their existence has been inferred from tiny doppler shifts in the light from the star. We…

Astrophysics · Physics 2008-11-26 R. Foot

In the past four decades a new type of astronomy has emerged, where instead of looking up into the sky "telescopes" are buried miles underground or deep under water or ice and search not for photons (that is, light), but rather for…

Astrophysics · Physics 2008-11-26 E. Waxman

Stars accrete near invisible hydrogen dominated agglomerates. This population, the `dark matter,' effects the nature of stars. Measurements show plasma streams impacting Earth, planets, Sun and stars. This mass-energy source contradicts…

Astrophysics · Physics 2007-05-23 Maurice Dubin , Robert K. Soberman

Extrasolar debris disks are the dust disks found around nearby main sequence stars arising from the break-up of asteroids and comets orbiting the stars. Far-IR surveys (e.g., with Herschel) showed that ~20% of stars host detectable dust…

Earth and Planetary Astrophysics · Physics 2020-01-22 Mark C. Wyatt

Stellar occultations provide a powerful tool to explore objects of the outer solar system. The Gaia mission now provides milli-arcsec accuracy on the predictions of these events and makes possible observations that were previously…

Earth and Planetary Astrophysics · Physics 2024-12-11 Bruno Sicardy , Felipe Braga-Ribas , Marc W. Buie , José Luis Ortiz , Françoise Roques

Exoplanet surveys have confirmed one of humanity's (and all teenagers') worst fears: we are weird. If our Solar System were observed with present-day Earth technology -- to put our system and exoplanets on the same footing -- Jupiter is the…

Earth and Planetary Astrophysics · Physics 2022-02-23 Sean N. Raymond , Andre Izidoro , Alessandro Morbidelli

Circumstellar disks have long been regarded as windows into planetary systems. The advent of high sensitivity, high resolution imaging in the submillimetre where both the solid and gas components of disks can be detected opens up new…

Earth and Planetary Astrophysics · Physics 2016-03-23 Brenda C. Matthews , JJ Kavelaars

We have conducted a novel search of most of the southern sky for nearby red dwarfs having low proper motions, with specific emphasis on those with proper motion < 0.18 arcsec yr-1, the lower cutoff of Luyten's classic proper motion catalog.…

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