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Related papers: Evidence for Two Populations of Classical Transnep…

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We investigate the long-term evolution of the inclinations of the known classical and resonant Kuiper belt objects (KBOs). This is partially motivated by the observed bimodal inclination distribution and by the putative physical differences…

Earth and Planetary Astrophysics · Physics 2015-05-28 Kathryn Volk , Renu Malhotra

We present the faintest mid ecliptic latitude survey in the second part of HST archival search for outer Solar System bodies. We report the discovery of 28 new trans-Neptunian objects and 1 small centaur (R ~ 2km) in the band 5{\circ} -…

Earth and Planetary Astrophysics · Physics 2015-05-30 Cesar I. Fuentes , David E. Trilling , Matthew J. Holman

We present three improved and five new mutual orbits of transneptunian binary systems (58534) Logos-Zoe, (66652) Borasisi-Pabu, (88611) Teharonhiawako-Sawiskera, (123509) 2000 WK183, (149780) Altjira, 2001 QY297, 2003 QW111, and 2003 QY90…

Earth and Planetary Astrophysics · Physics 2015-05-27 W. M. Grundy , K. S. Noll , F. Nimmo , H. G. Roe , M. W. Buie , S. B. Porter , S. D. Benecchi , D. C. Stephens , H. F. Levison , J. A. Stansberry

Asteroids that follow similar orbits may have a dynamical connection as their current paths could be the result of a past interaction with a massive perturber. The pair of extreme trans-Neptunian objects or ETNOs (474640) 2004 VN112-2013…

Earth and Planetary Astrophysics · Physics 2017-10-04 C. de la Fuente Marcos , R. de la Fuente Marcos , S. J. Aarseth

The dynamically cold component of the Kuiper Belt is host to a population of very widely separated, near-equal mass binary systems. Such binaries, representing the tail of the separation distribution of the more common, more tightly-bound…

Earth and Planetary Astrophysics · Physics 2012-07-04 Alex H. Parker

Recent photometric surveys of Trans-Neptunian Objects (TNOs) have revealed that the cold classical TNOs have distinct z-band color characteristics, and occupy their own distinct surface class. This suggested the presence of an absorption…

Earth and Planetary Astrophysics · Physics 2021-02-18 Tom Seccull , Wesley C. Fraser , Thomas H. Puzia

A current issue in the study of planetary nebulae with close binary central stars is the extent to which the binaries affect the shaping of the nebulae. Recent studies have begun to show a high coincidence rate between nebulae with…

Solar and Stellar Astrophysics · Physics 2016-12-07 Todd Hillwig , David Jones , Orsola De Marco , Howard Bond , Steve Margheim , David Frew

We have identified a binary companion to (42355) 2002 CR46 in our ongoing deep survey using the Hubble Space Telescope's High Resolution Camera. It is the first companion to be found around an object in a non-resonant orbit that crosses the…

Astrophysics · Physics 2009-11-11 K. S. Noll , H. F. Levison , W. M. Grundy , D. C. Stephens

We present results from a Hubble Space Telescope imaging search for low-mass binary and planetary companions to 33 nearby brown dwarfs with spectral types of T8-Y1. Our survey provides new photometric information for these faint systems,…

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…

The dependences of inclinations of orbits of secondaries in the discovered trans-Neptunian binaries on the distance between the primary and the secondary, on the eccentricity of orbits of the secondary around the primary, on the ratio of…

Earth and Planetary Astrophysics · Physics 2018-01-17 S. I. Ipatov

We have attempted to establish an observational evidence for presence of distant companions which may have acquired and/or absorbed the angular momentum during evolution of multiple systems thus facilitating or enabling formation of contact…

Astrophysics · Physics 2008-11-26 Theodor Pribulla , Slavek M. Rucinski

The Kepler Observatory offers unprecedented photometric precision (<1 mmag) and cadence for monitoring the central stars of planetary nebulae, allowing the detection of tiny periodic light curve variations, a possible signature of binarity.…

Solar and Stellar Astrophysics · Physics 2015-05-30 D. Douchin , G. H. Jacoby , O. De Marco , S. B. Howell , M. Kronberger

The 5:3 and 7:4 mean motion resonances of Neptune are at 42.3 and 43.7 au, respectively, and overlap with objects in the Classical trans-neptunian belt (Kuiper belt). We report the complete/partial lightcurves of 13 and 14 trans-Neptunian…

Earth and Planetary Astrophysics · Physics 2024-02-09 Audrey Thirouin , Scott S. Sheppard

In an effort to better understand the details of the stellar structure and evolution of metal poor stars, the Gemini North telescope was used on two occasions to take speckle imaging data of a sample of known spectroscopic binary stars and…

Among the 120 000 objects in the Hipparcos catalogue, only 235 were fitted with an orbital model. Besides these 235 original astrometric binaries, most Hipparcos entries with a known spectroscopic orbit (extrasolar planet or stellar…

Astrophysics · Physics 2007-05-23 D. Pourbaix , S. Jancart , A. Jorissen

We analyze albedo data obtained using the Herschel Space Observatory that reveal the existence of two distinct types of surface among midsized transneptunian objects. A color-albedo diagram shows two large clusters of objects, one redder…

The past two decades have seen a significant advancement in the detection, classification and understanding of exoplanets and binaries. This is due, in large part, to the increase in use of small-aperture telescopes (< 20 cm) to survey…

Solar and Stellar Astrophysics · Physics 2016-09-21 Ryan J. Oelkers , Lucas M. Macri , Jennifer L. Marshall , Darren L. DePoy , Diego G. Lambas , Carlos Colazo , Katelyn Stringer

Hubble Space Telescope observations between 2001 and 2010 resolved the binary components of the Cold Classical transneptunian object (79360) Sila-Nunam (provisionally designated 1997 CS29). From these observations we have determined the…