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We have calculated the coherence and detectable lifetimes of synthetic near-Earth object (NEO) families created by catastrophic disruption of a progenitor as it suffers a very close Earth approach. The closest or slowest approaches yield…

Earth and Planetary Astrophysics · Physics 2015-06-19 Eva Schunová , Robert Jedicke , Kevin J. Walsh , Mikael Granvik , Richard J. Wainscoat , Nader Haghighipour

We report on photometry and imaging of Comet 10P/Tempel 2 obtained at Lowell Observatory from 1983 through 2011. We measured a nucleus rotation period of 8.950 +/- 0.002 hr from 2010 September to 2011 January. This rotation period is longer…

Earth and Planetary Astrophysics · Physics 2015-06-11 Matthew M. Knight , David G. Schleicher , Tony L. Farnham , Edward W. Schwieterman , Samantha R. Christensen

We obtained extensive narrowband photoelectric photometry of Comet 21P/Giacobini-Zinner with observations spanning 33 years. The original data from 1985 (Schleicher et al. 1987) were re-reduced and are presented along with data from three…

Earth and Planetary Astrophysics · Physics 2022-04-27 David G. Schleicher

Much of the dynamical structure of the Kuiper belt can be explained if Neptune migrated over several AU, and/or if Neptune was scattered to an eccentric orbit during planetary instability. An outstanding problem with the existing formation…

Earth and Planetary Astrophysics · Physics 2015-08-19 David Nesvorny

Transiting planets in nearby young clusters offer the opportunity to study the atmospheres and dynamics of planets during their formative years. To this end, we focused on K2-25b -- a close-in ($P$=3.48 days), Neptune-sized exoplanet…

[Abridged] The detection of abundant O$_{2}$ ice at 1-10% with respect to H$_{2}$O ice in the comae of comets 1P/Halley and 67P/Churyumov-Gerasimenko motivated attempts to explain the origin of the high O$_{2}$ ice abundance. Recent…

Earth and Planetary Astrophysics · Physics 2019-01-16 Christian Eistrup , Catherine Walsh

The surprising discovery by the Rosetta spacecraft of molecular oxygen (O$_2$) in the coma of comet 67P/Churyumov-Gerasimenko (Bieler et al. 2015) challenged our understanding of the inventory of this volatile species on and inside bodies…

Earth and Planetary Astrophysics · Physics 2017-08-02 J. A. Kammer , S. A. Stern , G. R. Gladstone , L. A. Young , C. B. Olkin , A. Steffl , H. A. Weaver , K. Ennico

This paper presents the past evolution of the orbital elements of comet 67P/Churyumov-Gerasimenko, target of the Rosetta spacecraft. The gravitational orbit of the comet is affected by the sublimation of ice from the nucleus that triggers…

Earth and Planetary Astrophysics · Physics 2015-07-01 Lucie Maquet

A star passing within $\sim 10^4 \au$ of the Sun would trigger a comet shower that would reach the inner solar system about 0.18 Myr later. We calculate a prior probability of ~0.4% that a star has passed this close to the Sun but that the…

Astrophysics · Physics 2009-10-30 Jay A. Frogel , Andrew Gould

On 4 July 2005 at 05:52 UT, the impactor of NASA's Deep Impact (DI) mission crashed into comet 9P/Tempel 1 with a velocity of about 10 km/s. The material ejected by the impact expanded into the normal coma, produced by ordinary cometary…

Comet P/2019 LD2 has orbital elements currently resembling those of a Jupiter Trojan, and therefore superficially appears to represent a unique opportunity to study the volatile content and active behavior of a member of this population for…

Earth and Planetary Astrophysics · Physics 2020-09-02 Henry H. Hsieh , Alan Fitzsimmons , Bojan Novakovic , Larry Denneau , Aren N. Heinze

We present the analysis of the polarimetric and spectral data obtained for the dynamically new comet C/2012\,J1 (Catalina) when it was at a distance of 3.17~AU from the Sun. The observations were made at the prime focus of the 6-m BTA…

Earth and Planetary Astrophysics · Physics 2015-09-16 O. Ivanova , O. Shubina , A. Moiseev , V. Afanasiev

We present an interferometric search for large molecules, including methanol, methyl cyanide, ethyl cyanide, ethanol, and methyl formate in comets LINEAR (C/2002 T7) and NEAT (C/2001 Q4) with the Berkeley-Illinois-Maryland Association…

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…

We report the discovery of a pre-main-sequence, low-mass, double-lined, spectroscopic, eclipsing binary in the Orion star-forming region. We present our observations including radial velocities derived from optical high-resolution…

Astrophysics · Physics 2009-11-13 P. A. Cargile , K. G. Stassun , R. D. Mathieu

[Abridged] With a growing number of molecules observed in many comets, and an improved understanding of chemical evolution in protoplanetary disk midplanes, comparisons can be made between models and observations that could potentially…

Earth and Planetary Astrophysics · Physics 2019-09-11 Christian Eistrup , Catherine Walsh , Ewine F. van Dishoeck

We analyze findings of the Stardust mission that brought to the Earth dust from the 81P/Wild 2 coma. Just as the data of the Deep Impact mission to 9P/Tempel 1, they are at odds with the widely accepted condensation/sublimation comet…

Astrophysics · Physics 2008-11-26 Edward M. Drobyshevski

Main belt comets (MBCs) are a peculiar class of volatile-containing objects with comet-like morphology and asteroid-like orbits. However, MBCs are challenging targets to study remotely due to their small sizes and the relatively large…

Earth and Planetary Astrophysics · Physics 2019-11-20 B. Yang , E. Jehin , F. J. Pozuelos , Y. Moulane , Y. Shinnaka , C. Opitom , H. H. Hsieh , D. Hutsemékers , J. Manfroid

We present a series of observations of the return of activity in main-belt comet 238P/Read. Using data obtained in July and August 2010 when 238P appeared to be largely inactive, we find best-fit IAU phase function parameters of…

Earth and Planetary Astrophysics · Physics 2015-05-28 Henry H. Hsieh , Karen J. Meech , Jana Pittichova

Leo P is a low-luminosity dwarf galaxy discovered through the blind HI Arecibo Legacy Fast ALFA (ALFALFA) survey. The HI and follow-up optical observations have shown that Leo P is a gas-rich dwarf galaxy with active star formation, an…

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