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We use measurements from the Rosetta plasma consortium (RPC) Langmuir probe (LAP) and mutual impedance probe (MIP) to study the spatial distribution of low-energy plasma in the near-nucleus coma of comet 67P/Churyumov-Gerasimenko. The…

We used the UltraViolet-Optical Telescope on board Swift to systematically follow the dynamically new comet C/2013 A1 (Siding Spring) on its approach to the Sun. The comet was observed from a heliocentric distance of 4.5 AU pre-perihelion…

地球与行星天体物理 · 物理学 2015-06-24 Dennis Bodewits , Michael S. P. Kelley , Jian-Yang Li , Tony L. Farnham , Michael F. A'Hearn

We observed Comet C/Siding Spring using the Hubble Space Telescope (HST) during its close approach to Mars. The high spatial resolution images obtained through the F689M, F775W, and F845M filters reveal the characteristics of the dust coma.…

We study the development of activity in the incoming long-period comet C/2017 K2 over the heliocentric distance range 9 < r_H < 16 AU. The comet continues to be characterized by a coma of sub-millimeter and larger particles ejected at low…

地球与行星天体物理 · 物理学 2021-03-24 David Jewitt , Yoonyoung Kim , Max Mutchler , Jessica Agarwal , Jing Li , Harold Weaver

Molecular oxygen has been detected in the coma of comet 67P/Churyumov-Gerasimenko with abundances in the 1-10% range by the ROSINA-DFMS instrument on board the Rosetta spacecraft. Here we find that the radiolysis of icy grains in…

Recent spacecraft and radar observations have found that ~70 percent of short-period comet nuclei, mostly Jupiter-family comets (JFCs), have bilobate shapes (two masses connected by a narrow neck). This is in stark contrast to the shapes of…

地球与行星天体物理 · 物理学 2020-11-04 Taylor K. Safrit , Jordan K. Steckloff , Amanda S. Bosh , David Nesvorny , Kevin Walsh , Ramon Brasser , David A. Minton

Comet 49P/Arend-Rigaux is a well known low-activity Jupiter Family comet. Despite the low activity, we have witnessed outgassing activity in 1992, 2004, and 2012. In 2012 a broad tail-like feature (PA$\sim270^\circ, \sim2.3\times10^5$ km)…

We analyse the association between the NEAs 2021 PH27 and 2025 GN1, which share similar heliocentric Keplerian elements and the same taxonomic classification. First, we confirm the spectral similarity by getting independent colours…

地球与行星天体物理 · 物理学 2026-01-08 Albino Carbognani , Marco Fenucci , Toni Santana-Ros , Clara E. Martínez-Vázquez , Marco Micheli

Since 1950 when Oort published his paper on the structure of the cloud of comets it is believed that stars passing near this hypothetical cometary reservoir play an important role in the dynamical evolution of long period comets and…

地球与行星天体物理 · 物理学 2020-01-08 Rita Wysoczańska , Piotr A. Dybczyński , Małgorzata Królikowska

Comet C/2013 US10 (Catalina) was an dynamically new Oort cloud comet whose apparition presented a favorable geometry for observations near close Earth approach (~0.93au) at heliocentric distances ~2au when insolation and sublimation of…

地球与行星天体物理 · 物理学 2020-11-16 Charles E. Woodward , Diane H. Wooden , David E. Harker , Michael S. P. Kelley , Ray W. Russell , Daryl L. Kim

Molecular oxygen has been detected in the coma of comet 67P/Churyumov--Gerasimenko with a mean abundance of 3.80 $\pm$ 0.85\% by the ROSINA mass spectrometer on board the Rosetta spacecraft. To account for the presence of this species in…

地球与行星天体物理 · 物理学 2018-06-06 O. Mousis , T. Ronnet , J. I. Lunine , R. Maggiolo , P. Wurz , G. Danger , A. Bouquet

The (yet-to-be confirmed) discovery of a Neptune-sized moon around the ~3.2 Jupiter-mass planet in Kepler 1625 puts interesting constraints on the formation of the system. In particular, the relatively wide orbit of the moon around the…

地球与行星天体物理 · 物理学 2019-10-30 Adrian S. Hamers , Simon F. Portegies Zwart

We report the discovery of four dusty cometary tails around low mass stars in two young clusters belonging to the W5 star forming region. Fits to the observed emission profiles from 24 micron observations with the Spitzer Space Telescope…

天体物理学 · 物理学 2009-11-13 X. P. Koenig , L. E. Allen , S. J. Kenyon , K. Y. L. Su , Z. Balog

Our current understanding of split, Jupiter-family comets is reviewed. The focus is on what recent studies of comets have told us about the nature of the splitting phenomenon. The goal is to not repeat the information given in recent…

地球与行星天体物理 · 物理学 2009-07-29 Y. R. Fernandez

We present VLT/MUSE observations of comet 67P/Churyumov-Gerasimenko during its 2021 perihelion passage, from which we generated simultaneous maps of dust, [OI], C$_2$, NH$_2$, and CN comae across 12 pre- and post-perihelion epochs. These…

地球与行星天体物理 · 物理学 2025-07-21 Brian P. Murphy , Cyrielle Opitom , Colin Snodgrass , Sophie E. Deam , Léa Ferellec , Matthew Knight , Bin Yang , Vincent Okoth

We report results of intensive time-resolved imaging photometry and synoptic deep imaging of the comet C/2012 S1 (ISON) performed in February 2013. The data were obtained at the Wise Observatory in Israel (WO), at the Himalayan Chandra…

地球与行星天体物理 · 物理学 2024-07-02 Margarita Safonova , Noah Brosch , Shai Kaspi , David Polishook , R. Michael Rich , Firoza Sutaria , Jayant Murthy

One possible formation mechanism for Hot Jupiters is that high-eccentricity gas giants experience tidal interactions with their host star that cause them to lose orbital energy and migrate inwards. We study these types of tidal interactions…

The discovery of the transient Jupiter co-orbital comet P/2019 LD2 (ATLAS) drew significant interest. Not only will LD2 transition between being a Centaur and a Jupiter Family Comet (JFC) in 2063, the first time this process can be observed…

地球与行星天体物理 · 物理学 2024-04-15 Theodore Kareta , John W. Noonan , Kathryn Volk , Ryder H. Strauss , David Trilling

Jupiter Family Comets (JFCs), having orbital period less than 20 years, provide us with an opportunity to observe their activity and analyse the homogeneity in their coma composition over multiple apparitions. Comet 46P/Wirtanen with its…

地球与行星天体物理 · 物理学 2024-04-11 K. Aravind , Kumar Venkataramani , Shashikiran Ganesh , Emmanuel Jehin , Youssef Moulane

The asteroids are primitive solar system bodies which evolve both collisionally and through disruptions due to rapid rotation [1]. These processes can lead to the formation of binary asteroids [2-4] and to the release of dust [5], both…

地球与行星天体物理 · 物理学 2017-10-11 Jessica Agarwal , David Jewitt , Max Mutchler , Harold Weaver , Stephen Larson