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Related papers: Five New and Three Improved Mutual Orbits of Trans…

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We present Hubble Space Telescope observations of six binary transneptunian systems: 2000 QL251, 2003 TJ58, 2001 XR254, 1999 OJ4, (134860) 2000 OJ67, and 2004 PB108. The mutual orbits of these systems are found to have periods ranging from…

Astrophysics · Physics 2009-11-13 W. M. Grundy , K. S. Noll , M. W. Buie , S. D. Benecchi , D. C. Stephens , H. F. Levison

We have observed 1999 RZ253 with the Hubble Space Telescope at seven separate epochs and have fit an orbit to the observed relative positions of this binary. Two orbital solutions have been identified that differ primarily in the…

Astrophysics · Physics 2009-11-10 K. S. Noll , D. C. Stephens , W. M. Grundy , I. Griffin

We describe a strategy for scheduling astrometric observations to minimize the number required to determine the mutual orbits of binary transneptunian systems. The method is illustrated by application to Hubble Space Telescope observations…

The low-inclination component of the Classical Kuiper Belt is host to a population of extremely widely-separated binaries. These systems are similar to other Trans-Neptunian binaries (TNBs) in that the primary and secondary components of…

Earth and Planetary Astrophysics · Physics 2015-05-30 Alex H. Parker , JJ. Kavelaars , Jean-Marc Petit , Lynne Jones , Brett Gladman , Joel Parker

Mutual events of trans-Neptunian binaries (TNBs) provide rare opportunities to measure the physical and orbital properties of small bodies in the outer solar system. However, successful observations of these events have been limited by…

Earth and Planetary Astrophysics · Physics 2026-03-06 Benjamin Proudfoot , Will Grundy , Darin Ragozzine

The trans-neptunian object (58534) 1997 CQ$_{29}$ (a.k.a. Logos) is a resolved wide binary in the dynamically Cold Classical population. With Hubble Space Telescope resolved observations where the primary Logos is well separated from its…

Earth and Planetary Astrophysics · Physics 2025-04-23 Audrey Thirouin , Keith S. Noll , William M. Grundy , Scott S. Sheppard , Felicity Escarzaga , Brian Donnelly

A new Hubble Space Telescope observation of the 7:4 resonant transneptunian binary system (385446) Manw\"e has shown that, of two previously reported solutions for the orbit of its satellite Thorondor, the prograde one is correct. The orbit…

Earth and Planetary Astrophysics · Physics 2015-06-19 W. M. Grundy , S. D. Benecchi , S. B. Porter , K. S. Noll

As part of an ongoing study to determine the distribution of orbital parameters for massive binaries in the Cygnus OB2 Association, we present the orbital solutions for two new single-lined spectroscopic binaries, MT059 (O8V) & MT258 (O8V),…

Astrophysics · Physics 2009-11-13 Daniel C. Kiminki , M. Virgina McSwain , Henry A. Kobulnicky

We have measured the separations and position angles of the two components of the binary transneptunian object 1997 CQ29 at eight epochs. From these data we are able to constrain the orbit and mass of this binary system. The best fitting…

Astrophysics · Physics 2009-11-10 Keith S. Noll , Denise C. Stephens , Will M. Grundy , David J. Osip , Ian Griffin

We report the discovery and orbital solutions for two new OB binaries in the Cygnus OB2 Association, MT311 (B2V+B3V) and MT605 (B0.5V+B2.5:V). We also identify the system MT429 as a probable triple system consisting of a tight eclipsing…

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…

The discovery and characteristics of transneptunian binaries are reviewed. In the 20 years since their first discovery, a wealth of detail has emerged including the frequency of binaries in different populations, their relative sizes and…

Earth and Planetary Astrophysics · Physics 2020-02-19 Keith S. Noll , William M. Grundy , David Nesvorny , Audrey Thirouin

We have searched 101 Classical transneptunian objects for companions with the Hubble Space Telescope. Of these, at least 21 are binary. The heliocentric inclinations of the objects we observed range from 0.6-34 degrees. We find a very…

We present recent measurements of the orbital motion in the binaries, DF Tau and ZZ Tau, and in the triples, Elias 12, T Tau, and V853 Oph. We observed these systems with the Fine Guidance Sensors on the Hubble Space Telescope and with…

Astrophysics · Physics 2008-11-26 G. H. Schaefer , M. Simon , T. L. Beck , E. Nelan , L. Prato

We report here the discovery of an new near-equal mass Trans-Neptunian Binaries (TNBs) L5c02 and the and the putative detection of a second TNB (L4k12) among the year two and three detections of the Canada-France-Eclipic Plane Survey…

Earth and Planetary Astrophysics · Physics 2015-05-19 H. -W. Lin , J. J. Kavelaars , W. -H. Ip , B. J. Gladman , J. M. Petit , R. L. Jones , Joel Wm. Parker

The period, mass ratio, eccentricity, and other orbital parameters are fundamental for investigating binary star evolution. However, the number of binaries with known orbital parameters remains limited. Utilizing the LAMOST-MRS survey, we…

Solar and Stellar Astrophysics · Physics 2025-04-17 Sufen Guo , Mikhail Kovalev , Jiao Li , Guoliang Lu , Shi Jia , Zhenwei Li , Jiangdan Li , Jianping Xiong , Mingkuan Yang , Tongyu He , Xuefei Chen , Zhanwen Han

About 40 transneptunian binaries (TNBs) have fully determined orbits with about 10 others being solved except for breaking the mirror ambiguity. Despite decades of study almost all TNBs have only ever been analyzed with a model that assumes…

We present the spectroscopic orbits of eleven nearby, mid-to-late M dwarf binary systems in a variety of configurations: two single-lined binaries (SB1s), seven double-lined binaries (SB2s), one double-lined triple (ST2), and one…

We report the discovery of 24 spectroscopic binary companions to giant stars. We fully constrain the orbital solution for 6 of these systems. We cannot unambiguously derive the orbital elements for the remaining stars because the phase…

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