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From 1988 to 2016, several stellar occultations have been observed to characterize Pluto's atmosphere and its evolution (Meza et al, 2019). From each stellar occultation, an accurate astrometric position of Pluto at the observation epoch is…

Simple theoretical calculations have suggested that small body impacts onto Pluto's newly discovered small satellites, Nix and Hydra, are capable of generating time-variable rings or dust sheets in the Pluto system. Using HST/ACS data…

天体物理学 · 物理学 2008-11-26 A. J. Steffl , S. A. Stern

Seven rocky planets orbit the nearby dwarf star TRAPPIST-1, providing a unique opportunity to search for atmospheres on small planets outside the Solar System (Gillon et al., 2017). Thanks to the recent launch of JWST, possible atmospheric…

The atmosphere of Triton was probed directly by observing a ground-based stellar occultation on 6 October 2022. This rare event yielded 23 positive light curves collected from 13 separate observation stations contributing to our campaign.…

New Horizons observations suggest that CH4 on Pluto has a complex history, involving reservoirs of different composition, thickness and stability controlled by volatile processes occurring on different timescales. In order to interpret…

Keck near-infrared images of Neptune from UT 26 July 2007 show that the cloud feature typically observed within a few degrees of Neptune's south pole had split into a pair of bright spots. A careful determination of disk center places the…

地球与行星天体物理 · 物理学 2015-05-18 S. H. Luszcz-Cook , I. de Pater , M. Adamkovics , H. B. Hammel

We retrieve vertical and meridional variations of methane mole fraction in Titan's lower troposphere by re-analyzing near-infrared ground-based observations from 17 July 2014 UT (Adamkovics et al., 2016). We generate synthetic spectra using…

地球与行星天体物理 · 物理学 2017-02-22 Juan M. Lora , Mate Adamkovics

The search for clouds on the dayside of hot Jupiters has been disadvantaged due to hot Jupiters having a limited number of high quality space-based observations. To date, retrieval studies have found no evidence for grey clouds on the…

地球与行星天体物理 · 物理学 2023-08-09 Jake Taylor , Vivien Parmentier

Prompt neutrino fluxes due to the interactions of high-energy cosmic rays with the Earth's atmosphere are backgrounds in the search for high-energy neutrinos of galactic or extra-galactic origin performed by Very Large Volume Neutrino…

高能物理 - 唯象学 · 物理学 2016-02-29 M. V. Garzelli , S. Moch , G. Sigl

Approach images taken by the LORRI imaging system during the New Horizons spacecraft encounter have been used to determine the mean radii and shapes of Pluto and Charon. The primary observations are limb locations derived using three…

A population of discrete HI clouds in the halo of the inner Galaxy has been discovered in 21cm observations made with the Green Bank Telescope. The halo clouds are seen up to 1.5 kpc from the Galactic plane at many longitudes. Their…

天体物理学 · 物理学 2009-11-07 Felix J. Lockman

In this article I summarize the current state of knowledge about the composition of Titan's atmosphere, and our current understanding of the suggested chemistry that leads to that observed composition. I begin with our present knowledge of…

地球与行星天体物理 · 物理学 2024-03-26 Conor A. Nixon

Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars, and is strongly dependent on latitude. While most latitudes…

The atmospheres of exoplanets reveal all their properties beyond mass, radius, and orbit. Based on bulk densities, we know that exoplanets larger than 1.5 Earth radii must have gaseous envelopes, hence atmospheres. We discuss contemporary…

地球与行星天体物理 · 物理学 2017-01-04 Drake Deming , Sara Seager

Theoretical analysis and observational evidences indicate that a brown dwarf with effective temperature greater than 1400 K would have dust cloud in its atmosphere. In this letter, we show that dust scattering should yield polarized…

天体物理学 · 物理学 2009-11-07 Sujan Sengupta , Vinod Krishan

Ultra-hot Jupiters have recently attracted interest from observers and theoreticians alike, as they provide observationally accessible test cases. We apply a hierarchical modelling approach as a virtual laboratory to study cloud formation…

地球与行星天体物理 · 物理学 2020-01-08 Ch. Helling , N. Iro , L. Corrales , D. Samra , K. Ohno , M. K. Alam , M. Steinrueck , B. Lew , K. Molaverdikhani , R. J MacDonald , O. Herbort , P. Woitke , V. Parmentier

Several clues indicate that Titan's atmosphere has been depleted in methane during some period of its history, possibly as recently as 0.5-1 billion years ago. It could also happen in the future. Under these conditions, the atmosphere…

地球与行星天体物理 · 物理学 2015-06-22 Benjamin Charnay , François Forget , Gabriel Tobie , Christophe Sotin , Robin Wordsworth

In recent years, several potentially habitable, probably terrestrial exoplanets and exoplanet candidates have been discovered. The amount of CO2 in their atmosphere is of great importance for surface conditions and habitability. In the…

地球与行星天体物理 · 物理学 2015-06-12 Philip von Paris , J. Lee Grenfell , Pascal Hedelt , Heike Rauer , Franck Selsis , Barbara Stracke

Time-limited space missions may miss rare occurrences of very dense clouds of lunar dust. At the same time, the information provided by the Earth-based monitoring of the Moon during at least the last three centuries still remains unused. In…

空间物理 · 物理学 2025-01-29 Oleksiy V. Arkhypov , Maxim L. Khodachenko

The space probe 'New Horizon' was launched on 19th of January 2006 in order to study Pluto and its moons. Spacecraft will fly by Pluto as close as 12500 km in the middle of July 2015 and will get the most detailed images of Pluto and its…

地球与行星天体物理 · 物理学 2015-05-01 Alexander V. Devyatkin , Ekaterina A. Bashakova , Viacheslav Yu. Slesarenko