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The extent of formation of organic molecules in the comae of comets showing relatively high activity
DOI: 10.1016/j.icarus.2024.116374 Bibcode: 2025Icar..42716374A

Acharyya, Kinsuk; Ahmed, Sana

Comets are a rich reservoir of complex organic molecules. Ground and space-based observatories have recently greatly enhanced the cometary molecular inventory. Although these molecules' origin is believed to be the cometary nucleus, they can be partially synthesized in the coma. We studied organic molecules' nucleus versus coma origins for various…

2025 Icarus
Rosetta 1
Surface activity of H2O and CO2 on comet 103P/Hartley2 derived from EPOXI/HRI images
DOI: 10.1016/j.icarus.2025.116557 Bibcode: 2025Icar..43516557S

Tenishev, Valeriy; Fougere, Nicolas; Combi, Michael +3 more

On November 4, 2010, the EPOXI extended the mission of the Deep Impact spacecraft, flew by comet 103P/Hartley 2, and made a series of spectral images in both the infrared and the visible. The High-Resolution Instrument Infrared Spectrometer (HRI-IR) observed the comet and its surrounding coma, enabling maps in the light of the infrared emissions o…

2025 Icarus
Rosetta 0
Measurement of D/H and 13C/12C ratios in methane ice on Eris and Makemake: Evidence for internal activity
DOI: 10.1016/j.icarus.2023.115923 Bibcode: 2024Icar..41115923G

Lunine, J. I.; Emery, J. P.; Hammel, H. B. +13 more

James Webb Space Telescope's NIRSpec infrared imaging spectrometer observed the outer solar system dwarf planets Eris and Makemake in reflected sunlight at wavelengths spanning 1 through 5 µm. Both objects have high albedo surfaces that are rich in methane ice, with a texture that permits long optical path lengths through the ice for solar p…

2024 Icarus
Rosetta JWST 18
Sublimation and infrared spectral properties of ammonium cyanide
DOI: 10.1016/j.icarus.2024.116007 Bibcode: 2024Icar..41316007G

Gerakines, Perry A.; Yarnall, Yukiko Y.; Hudson, Reggie L.

The ammonium ion (NH4+) has been suggested to be present in interstellar ices and has been observed on the surfaces of planetary bodies using infrared (IR) spectroscopy as the primary means of identification. Evidence for several ammonium salts has also been found in the dust and surface ices of comet 67P/Churyumov-Gerasimenk…

2024 Icarus
Rosetta 3
First holistic modelling of meteoroid ablation and fragmentation: A case study of the Orionids recorded by the Canadian Automated Meteor Observatory
DOI: 10.1016/j.icarus.2023.115842 Bibcode: 2024Icar..40815842V

Vida, Denis; Brown, Peter G.; Campbell-Brown, Margaret +1 more

18 mm-sized Orionid meteoroids were captured in 2019 and 2020 by the Canadian Automated Observatory's mirror tracking system. Meteor position measurements were made to an accuracy of ∼1m and the meteors were tracked to a limiting magnitude of about + 7 . 5 at the faintest point. The trajectory estimation shows the intrinsic physical dispersion of …

2024 Icarus
Rosetta 3
Comets, sliding of surface dust on illuminated surfaces
DOI: 10.1016/j.icarus.2023.115861 Bibcode: 2024Icar..41015861K

Kossacki, Konrad J.; Wesołowski, Marcin; Mikołajków, Tomasz +1 more

In our paper we presented the results of our laboratory experiments dealing with the formation and sliding of the desiccated nonvolatile granular material down the samples of potential cometary analogs. The studied samples were composed of porous aggregates containing water ice, quartz sand and charcoal. Their surfaces were initially free of desic…

2024 Icarus
Rosetta 2
New gravity field of comet 67P/C-G based on Rosetta's Doppler and optical data
DOI: 10.1016/j.icarus.2024.116284 Bibcode: 2024Icar..42416284L

Marty, Jean-Charles; Jorda, Laurent; Le Maistre, Sebastien +3 more

The gravity field of a celestial body gives valuable insights into its fundamental properties such as its density and internal structure. The Doppler data collected by the Radio-Science Investigation (RSI) experiment of the Rosetta mission were previously used to determine the gravity field of comet 67P/Churyumov–Gerasimenko up to degree 2 (Pätzol…

2024 Icarus
Rosetta 1
Modeling the plasma composition of 67P/C-G at different heliocentric distances
DOI: 10.1016/j.icarus.2024.116253 Bibcode: 2024Icar..42216253A

Ahmed, Sana; Soni, Vikas

The Rosetta spacecraft accompanied the comet 67P/C-G for nearly 2 years, collecting valuable data on the neutral and ion composition of the coma. The Rosetta Plasma Consortium (RPC) provided continuous measurements of the in situ plasma density while ROSINA-COPS monitored the neutral composition. In this work, we aim to estimate the composition of…

2024 Icarus
Rosetta 1
Common origin of trapped volatiles in oxidized icy moons and comets
DOI: 10.1016/j.icarus.2024.115944 Bibcode: 2024Icar..41115944O

Johnson, Robert E.; Oza, Apurva V.

Following spacecraft encounters with comets 67P/C-G and 1P/Halley, it was surprising that O2, expected to be a very minor species in their comas, was observed to outgas at a few percent abundance during their ice sublimation phases. This challenged the direct connection suggested between comets and material in the interstellar medium (I…

2024 Icarus
Rosetta 0
A race against the clock: Constraining the timing of cometary bombardment relative to Earth's growth
DOI: 10.1016/j.icarus.2023.115754 Bibcode: 2023Icar..40615754J

Nesvorný, David; Avice, Guillaume; Raymond, Sean N. +3 more

Comets are considered a potential source of inner solar system volatiles, but the timing of this delivery relative to that of Earth's accretion is still poorly understood. Measurements of xenon isotopes in comet 67P/Churyumov-Gerasimenko revealed that comets partly contributed to the Earth's atmosphere. However, there is no conclusive evidence of …

2023 Icarus
Rosetta 2