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20122026
most citedOSSOS. VII. 800+ trans-Neptunian objects - the complete data release

159 citations · 2.6k across the 74 of their papers we have counts for

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astro-ph.EP2026

Col-OSSOS: Investigating the Origins of Different Surfaces in the Primordial Kuiper Belt

Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser +12

The Colours of the Outer Solar System Origins Survey (Col-OSSOS) measured the optical/NIR colours of a brightness-complete sample of Trans-Neptunian Objects (TNOs). Like previous s…

astro-ph.EP2025★ 6 cited

Discovery and dynamics of a Sedna-like object with a perihelion of 66 au

Ying-Tung Chen, Patryk Sofia Lykawka, Yukun Huang +30

Trans-Neptunian objects (TNOs) with large perihelion distances ( au) and semi-major axes ( au) provide insights into the early evolution of the solar system and th…

astro-ph.EP2025

An Extremely Deep Rubin Survey to Explore the Extended Kuiper Belt and Identify Objects Observable by New Horizons

JJ Kavelaars, Marc W. Buie, Wesley C. Fraser +22

A proposed Vera C. Rubin Observatory Deep Drilling micro-survey of the Kuiper Belt will investigate key properties of the distant solar system. Utilizing 30 hours of Rubin time acr…

astro-ph.EP2023★ 2 cited

Ejecta Evolution Following a Planned Impact into an Asteroid: The First Five Weeks

Theodore Kareta, Cristina Thomas, Jian-Yang Li +85

The impact of the DART spacecraft into Dimorphos, moon of the asteroid Didymos, changed Dimorphos' orbit substantially, largely from the ejection of material. We present results fr…

astro-ph.EP2023★ 26 cited

The hot main Kuiper belt size distribution from OSSOS

Jean-Marc Petit, Brett Gladman, J. J. Kavelaars +4

Using the absolute detection calibration and abundant detections of the OSSOS (Outer Solar System Origin Survey) project, we provide population measurements for the main Kuiper Bel…

astro-ph.EP2023★ 16 cited

The Galactic Interstellar Object Population: A Framework for Prediction and Inference

Matthew J. Hopkins, Chris Lintott, Michele T. Bannister +2

The Milky Way is thought to host a huge population of interstellar objects (ISOs), numbering approximately around the Sun, which are formed and shaped by…

astro-ph.EP2023★ 10 cited

OSSOS. XXIX. The Population and Perihelion Distribution of the Detached Kuiper Belt

Matthew Beaudoin, Brett Gladman, Yukun Huang +4

The detached transneptunian objects (TNOs) are those with semimajor axes beyond the 2:1 resonance with Neptune, which are neither resonant nor scattering. Using the detached sample…

astro-ph.EP2023★ 2 cited

OSSOS: XXVII. Population Estimates for Theoretically Stable Centaurs Between Uranus and Neptune

Rosemary C. Dorsey, Michele T. Bannister, Samantha M. Lawler +1

We calculate the upper bounds of the population of theoretically stable Centaur orbits between Uranus and Neptune. These small bodies are on low-eccentricity, low-inclination orbit…

astro-ph.EP2023★ 79 cited

Tuning the Legacy Survey of Space and Time (LSST) Observing Strategy for Solar System Science

Megan E. Schwamb, R. Lynne Jones, Peter Yoachim +27

The Vera C. Rubin Observatory is expected to start the Legacy Survey of Space and Time (LSST) in early to mid-2025. This multi-band wide-field synoptic survey will transform our vi…

astro-ph.EP2023★ 119 cited

Ejecta from the DART-produced active asteroid Dimorphos

Jian-Yang Li, Masatoshi Hirabayashi, Tony L. Farnham +61

Some active asteroids have been proposed to be the result of impact events. Because active asteroids are generally discovered serendipitously only after their tail formation, the p…

astro-ph.EP2022

The LCO Outbursting Objects Key Project: Overview and Year 1 Status

Tim Lister, Michael S. P. Kelley, Carrie E. Holt +32

The LCO Outbursting Objects Key (LOOK) Project uses the telescopes of the Las Cumbres Observatory (LCO) Network to: (1) to systematically monitor a sample of Dynamically New Comets…

astro-ph.EP2022

Col-OSSOS: Evidence for a compositional gradient inherited from the protoplanetary disk?

Michael Marsset, Wesley C. Fraser, Megan E. Schwamb +7

In the present-day Kuiper Belt, the number of compositional classes and the orbital distributions of these classes hold important cosmogonic implications for the Solar System. In a…

astro-ph.EP2022★ 2 cited

Col-OSSOS: The Two Types of Kuiper Belt Surfaces

Wesley C. Fraser, Rosemary E. Pike Michael Marsset, Megan E. Schwamb +10

The Colours of the Outer Solar System Origins Survey (Col-OSSOS) has gathered high quality, near-simultaneous (g-r) and (r-J) colours of 92 Kuiper Belt Objects (KBOs) with (u-g) an…

astro-ph.EP2022

Col-OSSOS: The Distribution of Surface Classes in Neptune's Resonances

Rosemary E. Pike, Wesley C. Fraser, Kathryn Volk +9

The distribution of surface classes of resonant trans-Neptunian objects (TNOs) provides constraints on the protoplanetesimal disk and giant planet migration. To better understand t…

astro-ph.EP2022

OSSOS XXV: Large Populations and Scattering-Sticking in the Distant Transneptunian Resonances

B. L. Crompvoets, S. M. Lawler, K. Volk +8

There have been 77 TNOs discovered to be librating in the distant transneptunian resonances (beyond the 2:1 resonance, at semimajor axes greater than 47.7~AU) in four well-characte…

astro-ph.EP2021

Col-OSSOS: Probing Ice Line/Color Transitions within the Kuiper Belt's Progenitor Populations

Laura E. Buchanan, Megan E. Schwamb, Wesley C. Fraser +15

Dynamically excited objects within the Kuiper belt show a bimodal distribution in their surface colors, and these differing surface colors may be a tracer of where these objects fo…

astro-ph.EP2021★ 5 cited

OSSOS. XXIII. 2013 VZ70 and the Temporary Coorbitals of the Giant Planet

Mike Alexandersen, Sarah Greenstreet, Brett J. Gladman +8

We present the discovery of 2013 VZ70, the first known horseshoe coorbital companion of Saturn. Observed by the Outer Solar System Origins Survey (OSSOS) for 4.5 years, the orbit o…

astro-ph.EP2021

OSSOS finds an Exponential Cutoff in the Size Distribution of the Cold Classical Kuiper belt

JJ Kavelaars, Jean-Marc Petit, Brett Gladman +5

The cold main classical Kuiper Belt consists of those non-resonant small solar system bodies with low orbital inclinations and orbital semi-major axes between 42.4 and 47.7 au. The…

astro-ph.EP2021★ 22 cited

Collision Probabilities in the Edgeworth-Kuiper belt

Abedin Y. Abedin, JJ Kavelaars, Sarah Greenstreet +8

Here, we present results on the intrinsic collision probabilities, , and range of collision speeds, , as a function of the heliocentric distance, , in the trans-Neptu…

astro-ph.EP2021

Col-OSSOS: The Distinct Colour Distribution of Single and Binary Cold Classical KBOs

Wesley C. Fraser, Susan D. Benecchi, JJ Kavelaars +11

The cold classical Kuiper Belt Objects (KBOs) possess a high, binary fraction. Widely separated and dynamically fragile, these binary systems have been useful in trac…

astro-ph.EP2020★ 50 cited

OSSOS XX: The Meaning of Kuiper Belt Colors

David Nesvorny, David Vokrouhlicky, Mike Alexandersen +9

Observations show that 100-km-class Kuiper belt objects (KBOs) can be divided in (at least) two color groups, hereafter red (R, g-i<1.2) and very red (VR, g-i>1.2), reflecting a di…

astro-ph.EP2020★ 13 cited

OSSOS: The Eccentricity and Inclination Distributions of the Stable Neptunian Trojans

Hsing Wen Lin, Ying-Tung Chen, Kathryn Volk +10

The minor planets on orbits that are dynamically stable in Neptune's 1:1 resonance on Gyr timescales were likely emplaced by Neptune's outward migration. We explore the intrinsic l…

astro-ph.EP2020

Col-OSSOS: Compositional homogeneity of three Kuiper belt binaries

Michael Marsset, Wesley C. Fraser, Michele T. Bannister +10

The surface characterization of Trans-Neptunian Binaries (TNBs) is key to understanding the properties of the disk of planetesimals from which these objects formed. In the optical…

astro-ph.EP2020★ 16 cited

Interstellar comet 2I/Borisov as seen by MUSE: C, NH and red CN detections

Michele T. Bannister, Cyrielle Opitom, Alan Fitzsimmons +11

We report the clear detection of C and of abundant NH in the first prominently active interstellar comet, 2I/Borisov. We observed 2I on three nights in November 2019 at opt…