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We present deep imaging observations of activated asteroid P/2016 G1 (PANSTARRS) using the 10.4m Gran Telescopio Canarias (GTC) from late April to early June 2016. The images are best interpreted as the result of a relatively short-duration…

Earth and Planetary Astrophysics · Physics 2016-08-03 Fernando Moreno , Javier Licandro , Antonio Cabrera-Lavers , Francisco J. Pozuelos

The absolute magnitude and perihelion distributions of long-period comets are derived, using data from the Lincoln Near-Earth Asteroid Research (LINEAR) survey. The results are surprising in three ways. Firstly, the flux of comets through…

Astrophysics · Physics 2016-08-30 P. J. Francis

Long period comet C/2014 B1 (Schwartz) exhibits a remarkable optical appearance, like that of a discus or bi-convex lens viewed edgewise. Our measurements in the four years since discovery reveal a unique elongated dust coma whose…

Earth and Planetary Astrophysics · Physics 2019-02-20 David Jewitt , Yoonyoung Kim , Jane Luu , Ariel Graykowski

Data on perihelion fragmentation of the Great September Comet of 1882 (C/1882 R1), a prominent member of the Kreutz sungrazer system, are employed to estimate the size of the nucleus along the radius vector at the time of splitting. The…

Earth and Planetary Astrophysics · Physics 2021-10-22 Zdenek Sekanina

Cliff collapses on Comet 67P/Churyumov-Gerasimenko expose relatively pristine nucleus matter and offer rare opportunities to characterise ice-rich comet material. Here, Microwave Instrument for \emph{Rosetta} Orbiter (MIRO) observations of…

Earth and Planetary Astrophysics · Physics 2024-04-22 Björn J. R. Davidsson

We present our results for comet (ISON). Our results were obtained with amateur telescopes observing from the ground, before and after the comet had passed conjunction with the Sun in August 2013. We measured a mean radius of 830 +- 245 m,…

Solar and Stellar Astrophysics · Physics 2014-05-14 Toni Scarmato

The recent close approach of comet C/2020 F3 (NEOWISE) allowed us to study the morphology of its inner coma. From the measurement of the dust ejection velocityon spiral structures expanding around the nucleus, we estimated a mean…

Earth and Planetary Astrophysics · Physics 2021-09-07 F. Manzini , V. Oldani , P. Ochner , E. Barbotin , L. R. Bedin , R. Behrend , G. Fardelli

We report a new observation of the Jupiter-family comet 209P/LINEAR during its 2014 return. The comet is recognized as a dust source of a new meteor shower, the May Camelopardalids. 209P/LINEAR was apparently inactive at a heliocentric…

P/2010 A2 is an object on an asteroidal orbit that was observed to have an extended tail or debris trail in January 2010. In this work, we fit the outburst of P/2010 A2 with a conical burst model, and verify previous suspicions that this…

Earth and Planetary Astrophysics · Physics 2015-06-11 Jan Kleyna , Olivier Hainaut , Karen Meech

Aims. We aim to constrain the size and porosity of ejected dust particles from comet 252P/LINEAR and their evolution near the perihelion via near-infrared multiband polarimetry. A close approach of the comet to the Earth in March 2016…

Earth and Planetary Astrophysics · Physics 2019-09-18 Y. G. Kwon , M. Ishiguro , J. Kwon , D. Kuroda , M. Im , C. Choi , M. Tamura , T. Nagayama , N. Kawai , J. -I. Watanabe

Jupiter-family comet (JFC) P/2021 HS (PANSTARRS) only exhibits a coma within a few weeks of its perihelion passage at 0.8~au, which is atypical for a comet. Here we present an investigation into the underlying cause using serendipitous…

Comet P/2010A2 LINEAR is a good candidate for membership with the Main Belt Comet family. It was observed with several telescopes (ESO NTT, La Silla; Gemini North, Mauna Kea; UH 2.2m, Mauna Kea) from 14 Jan. until 19 Feb. 2010 in order to…

Earth and Planetary Astrophysics · Physics 2015-06-03 O. R. Hainaut , J. Kleyna , G. Sarid , B. Hermalyn , A. Zenn , K. J. Meech , P. H. Schultz , H. Hsieh , G. Trancho , J. Pittichová , B. Yang

Photometric and spectroscopic observations of five nearly parabolic comets with eccentricity larger than 0.99 at heliocentric distances greater than 4 AU were performed. No molecular emission was observed for any studied comet and the…

According to our common understandings, the original surface of a short-period comet nucleus has been lost by sublimation processes during its close approaches to the Sun. Sublimation results in the formation of a dust mantle on the…

State-of-the-art long-term solar system integrations include several second order effects such as the Sun's quadrupole moment J2 and a contribution from asteroids (plus the Moon and general relativity). We recently showed that including 10…

Earth and Planetary Astrophysics · Physics 2025-05-02 Richard E. Zeebe , Ilja J. Kocken

The Centaurs are recent escapees from the Kuiper belt that are destined either to meet fiery oblivion in the hot inner regions of the Solar system or to be ejected to the interstellar medium by gravitational scattering from the giant…

Earth and Planetary Astrophysics · Physics 2009-11-13 David Jewitt

Short-period comet P/2010 H2 (Vales) underwent a significant outburst of $>7.5$~mag in 2010 and has not been detected since that apparition. Here we report our recovery attempt of P/Vales using the 4.3-m Lowell Discovery Telescope (LDT)…

Earth and Planetary Astrophysics · Physics 2026-03-18 Quanzhi Ye , Tony L. Farnham , Perry Cai , Lori Feaga

On 31 August 2019, an interstellar comet was discovered as it passed through the Solar System (2I/Borisov). Based on initial imaging observations, 2I/Borisov appeared to be completely similar to ordinary Solar System comets - an unexpected…

Earth and Planetary Astrophysics · Physics 2021-05-20 Piotr Guzik , Michał Drahus

Solar system object P/2010 A2 is the first-noticed example of the aftermath of a recently disrupted asteroid, probably resulting from a collision. Nearly a year elapsed between its inferred initiation in early 2009 and its eventual…

Earth and Planetary Astrophysics · Physics 2015-05-28 David Jewitt , Joseph S. Stuart , Jing Li

We observed comet C/2012 S1 (ISON) during six nights in February 2013 when it was at 4.8 AU from the sun. At this distance and time the comet was not very active and it was theoretically possible to detect photometric variations likely due…