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Comet 73P-B/Schwassmann-Wachmann 3 was observed with IRCS/Subaru at geocentric distance of 0.074 AU on UT 10 May 2006. Multiple H2O emission lines were detected in non-resonant fluorescence near 2.9 microns. No significant variation in…

The cosmological origin of carbon, the fourth most abundant element in the Universe, is not well known and matter of heavy debate. We investigate the behavior of C/O to O/H in order to constrain the production mechanism of carbon. We…

星系天体物理 · 物理学 2017-10-04 Maria A. Peña-Guerrero , Claus Leitherer , Selma de Mink , Aida Wofford , Lisa Kewley

A morphological and photometric analysis of the naked-eye long-period comet C/2022 E3 (ZTF) before perihelion is presented in this study. The observation images taken by the Zwicky Transient Facility survey telescope from July 2022 to…

地球与行星天体物理 · 物理学 2024-05-27 Bin Liu , Xiaodong Liu

Recently the ROSINA mass spectrometer suite on board the European Space Agency's Rosetta spacecraft discovered an abundant amount of molecular oxygen, O2, in the coma of Jupiter family comet 67P/Churyumov-Gerasimenko of O2/H2O =…

地球与行星天体物理 · 物理学 2015-12-08 Martin Rubin , Kathrin Altwegg , Ewine F. van Dishoeck , Gerhard Schwehm

Comet 12P/Pons-Brook exhibited multiple large and minor outbursts in 2023 on its way to its 2024 perihelion, as it has done during its previous apparitions. We obtained long-slit optical spectra of the comet in 2023 August and 2023 November…

地球与行星天体物理 · 物理学 2024-10-31 Lea Ferellec , Cyrielle Opitom , Abbie Donaldson , Johan P. U. Fynbo , Rosita Kokotanekova , Michael S. P. Kelley , Tim Lister

We discuss the morphology and spectrophotometry of 5 comets visible in August, 2001. We decompose comae into coma profiles and azimuthally renormalized images, in which general and local features are quantitatively comparable. Comet…

天体物理学 · 物理学 2009-11-07 Gy. M. Szabo , L. L. Kiss , K. Sarneczky , K. Sziladi

We present optical and near-infrared (NIR) observations of the outbursting, Halley-type comet 12P/Pons-Brooks. Three NIR spectra were obtained during two outbursts in October and November 2023, with the 3-meter Infrared Telescope Facility…

地球与行星天体物理 · 物理学 2026-05-01 Ruining Zhao , Bin Yang , Michael S. P. Kelley , Silvia Protopapa , Aigen Li , Yang Huang , Jifeng Liu

Comet 7P/Pons-Winnecke was observed from the Calar Alto Observatory (Spain) for four months during the 2021 inbound apparition. Broad-band visible images were taken between 1.71 and 1.25 AU pre-perihelion, while long-slit spectrophotometric…

地球与行星天体物理 · 物理学 2025-03-18 Irene Mariblanca-Escalona , Luisa M. Lara , Fernando Moreno , Pedro J. Gutiérrez , Marçal Evangelista-Santana

Hyperactive comets are a small group of comets whose activity are higher than expected. They seem to emit more water than they should based on the size of their nucleus and comet 46P/Wirtanen is one of them. Investigating its activity and…

Chemical equilibrium considerations suggest that, assuming solar elemental abundances, carbon on HD 209458b is sequestered primarily as carbon monoxide (CO) and methane (CH4). The relative mole fractions of CO(g) and CH4(g) in chemical…

天体物理学 · 物理学 2008-11-26 Curtis S. Cooper , Adam P. Showman

176P/LINEAR is a member of the new cometary class known as main-belt comets (MBCs). It displayed cometary activity shortly during its 2005 perihelion passage that may be driven by the sublimation of sub-surface ices. We have therefore…

The release of volatiles from comets is usually from direct sublimation of ices on the nucleus, but for very or hyper-active comets other sources have to be considered to account for the total production rates. In this work, we present new…

地球与行星天体物理 · 物理学 2023-04-13 Theodore Kareta , John W. Noonan , Walter M. Harris , Alessondra Springmann

Gas-phase molecules in cometary atmospheres (comae) originate primarily from (1) outgassing by the nucleus, (2) sublimation of icy grains in the near-nucleus coma, and (3) coma (photo-)chemical processes. However, the majority of cometary…

Isotopic measurements of Solar System bodies provide a primary paradigm within which to understand the origins and histories of planetary materials. The D/H ratio in particular, helps reveal the relationship between (and heritage of)…

We report results from an analysis of the volatile composition and evolution of main-belt comet (MBC) 133P/Elst-Pizarro using JWST NIRSpec and NIRCam observations and ground-based observations during its 2024 active apparition, and also…

Observations of the sungrazing comet C/2012 S1 (ISON) were carried out using the Atacama Large Millimeter/submillimeter Array (ALMA) at a heliocentric distance of 0.58-0.54 AU (pre-perihelion) on 2013 November 16-17. Temporally resolved…

Comet C/2020 F3 (NEOWISE) was the brightest comet in the northern hemisphere since C/1995 O1 (Hale-Bopp), providing a unique opportunity to study its composition and spatial distribution of emissions. We conducted narrow-band photometry and…

地球与行星天体物理 · 物理学 2025-09-17 K. Aravind , E. Jehin , S. Hmmidouch , M. Vander Donckt , S. Ganesh , P. Rousselot , P. Hardy , D. Sahu , J. Manfroid , Z. Benkhaldoun

The D/H ratio in cometary water is believed to be an important indicator of the conditions under which icy planetesimals formed and can provide clues to the contribution of comets to the delivery of water and other volatiles to Earth.…

We present the first detection of carbon monoxide (CO) in a damped Lyman-alpha system (DLA) at z_abs =2.41837 toward SDSS J143912.04+111740.5. We also detected H_2 and HD molecules. The measured total column densities (in log units) of H I,…

天体物理学 · 物理学 2020-12-23 R. Srianand , P. Noterdaeme , C. Ledoux , P. Petitjean

Comet 133P/Elst-Pizarro is the first-known and currently best-characterised member of the main-belt comets, a recently-identified class of objects that exhibit cometary activity but which are dynamically indistinguishable from main-belt…

地球与行星天体物理 · 物理学 2015-05-14 Henry H. Hsieh , David Jewitt , Pedro Lacerda , Stephen C. Lowry , Colin Snodgrass