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Related papers: Note on the dynamical evolution of C/2017 K2 PANST…

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The 2023 perihelion passage of comet C/2022 E3 (ZTF) afforded an opportunity to measure the abundances and spatial distributions of coma volatiles in an Oort cloud comet at high spatial resolution near its close approach to Earth…

We report on the catastrophic disintegration of P/2016 G1 (PANSTARRS), an active asteroid, in April 2016. Deep images over three months show that object is constituted by a central concentration of fragments surrounded by an elongated coma,…

Context. The dynamical evolution of near-parabolic comets strongly depends on the starting values of the orbital elements derived from the positional observations. In addition, when drawing conclusions about the origin of these objects, it…

Earth and Planetary Astrophysics · Physics 2014-09-05 Małgorzata Królikowska

Context. Kepler-17 is a G2V sun-like star accompanied by a transiting planet with a mass of ~2.5 Jupiter masses and an orbital period of 1.486 d, recently discovered by the Kepler space telescope. This star is highly interesting as a young…

Earth and Planetary Astrophysics · Physics 2015-06-11 Aldo S. Bonomo , Antonino F. Lanza

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

The N$_2$ and CO-rich and water-depleted comet C/2016 R2 (Pan-STARRS) (hereafter `C/2016 R2') is a unique comet for detailed spectroscopic analysis. We aim to explore the associated photochemistry of parent species, which produces different…

Earth and Planetary Astrophysics · Physics 2020-03-25 S. Raghuram , D. Hutsemékers , C. Opitom , E. Jehin , A. Bhardwaj , J. Manfroid

Recent observations of the long period comet C/2016 R2 (PanSTARRS) indicate an unusually high N2/CO abundance ratio, typically larger than 0.05, and at least 2-3 times higher than the one measured in 67P/Churyumov-Gerasimenko. Another…

Gateway Centaur and Jupiter co-orbital P/2019 LD2 (ATLAS) (Sarid et al. 2019) provides the first opportunity to observe the migration of a Solar System small body from a Centaur orbit to a Jupiter Family Comet (JFC) four decades from now…

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

We present an analysis of comet activity based on the Spitzer Space Telescope component of the Survey of the Ensemble Physical Properties of Cometary Nuclei. We show that the survey is well suited to measuring the activity of Jupiter-family…

Passing stars can perturb the Oort Cloud, triggering comet showers and potentially extinction events on Earth. We combine velocity measurements for the recently discovered, nearby, low-mass binary system WISE J072003.20-084651.2 ("Scholz's…

We present observations using the Baade Magellan and Canada-France-Hawaii telescopes showing that main-belt comet 324P/La Sagra, formerly known as P/2010 R2, has become active again for the first time since originally observed to be active…

Earth and Planetary Astrophysics · Physics 2015-10-07 Henry H. Hsieh , Scott S. Sheppard

The recent observations show that comet C/2016 R2 (Pan-Starrs) has a unique and peculiar composition when compared with several other comets observed at 2.8 au heliocentric distance. Assuming solar resonance fluorescence is the only…

Earth and Planetary Astrophysics · Physics 2021-01-06 Susarla Raghuram , Anil Bhardwaj , Damien Hutsemékers , Cyrielle Opitom , Jean Manfroid , Emmanuel Jehin

Recent measurements carried out at comet 67P/C-G with the ${\it Rosetta}$ probe revealed that molecular oxygen, O$_2$, is the fourth most abundant molecule in comets. Models show that O$_2$ is likely of primordial nature, coming from the…

We report our new analysis of Oort-cloud comet C/2020 T2 (Palomar) (T2) observed at 2.06 au from the Sun (phase angle of 28.5 deg) about two weeks before perihelion. T2 lacks a significant dust tail in scattered light, showing a strong…

Earth and Planetary Astrophysics · Physics 2022-12-14 Yuna Grace Kwon , Joseph R. Masiero , Johannes Markkanen

C/2002 CE$_{10}$ is an object in a retrograde elliptical orbit with Tisserand parameter $-0.853$ indicating a likely origin in the Oort Cloud. It appears to be a rather inactive comet since no coma and only a very weak tail was detected…

Earth and Planetary Astrophysics · Physics 2018-02-28 Tomohiko Sekiguchi , Seidai Miyasaka , Budi Dermawan , Thomas Mueller , Naruhisa Takato , Junichi Watanabe , Hermann Boehnhardt

We present JWST NIRSpec and NIRCam observations of 457P/Lemmon-PANSTARRS, a main-belt comet that displayed activity around its 2020 perihelion and that was observed to regain activity during its 2024 perihelion by a ground-based observing…

We present the polarimetric results and analysis of comet C/2012 L2 (LINEAR) observed at 31$^\circ$.1 phase angle before perihelion passage. The observations of the comet were carried out using ARIES Imaging Polarimeter (AIMPOL) mounted on…

Earth and Planetary Astrophysics · Physics 2014-12-01 P. DebRoy , H. S. Das , Biman J. Medhi

The SRa02 of the CoRoT space mission for Asteroseismology was partly devoted to stars belonging to the Mon OB2 association. An intense monitoring was performed on Plaskett's Star (HD47129) and the unprecedented quality of the light curve…

Solar and Stellar Astrophysics · Physics 2015-05-20 L. Mahy , E. Gosset , F. Baudin , G. Rauw , M. Godart , T. Morel , P. Degroote , C. Aerts , R. Blomme , J. Cuypers , A. Noels , E. Michel , A. Baglin , M. Auvergne , C. Catala , R. Samadi

We present mid-infrared observations of comet P/2016 BA14 (PANSTARRS), which were obtained on UT 2016 March 21.3 at heliocentric and geocentric distances of 1.012 au and 0.026 au, respectively, approximately 30 hours before its closest…

Earth and Planetary Astrophysics · Physics 2021-04-14 Takafumi Ootsubo , Hideyo Kawakita , Yoshiharu Shinnaka
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