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相关论文: Active Cryovolcanism on Europa?

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We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption at 16.5S jovigraphic latitude had been reported by the…

The location of a repeat plume detected at Europa is found to be coincident with the strongest ionosphere detection made by Galileo radio occultation in 1997.

地球与行星天体物理 · 物理学 2017-11-13 Melissa A. McGrath , William B. Sparks

We present maps of surface composition of Europa's anti-jovian hemisphere acquired using high spatial resolution IFU multi-spectral data from the SPHERE instrument on the Very Large Telescope (0.95 to 1.65$\mu$m) and the NIMS instrument on…

地球与行星天体物理 · 物理学 2022-09-07 Oliver King , Leigh N Fletcher , Nicolas Ligier

Jupiter's moon Europa has a thin icy crust which is decoupled from the mantle by a subsurface ocean. The crust thus responds to tidal forcing as a deformed membrane, cold at the top and near melting point at the bottom. In this paper I…

地球物理 · 物理学 2015-06-01 Mikael Beuthe

The relatively warm climate found in the North- Western Europe is due to the gulf stream that circulates warm saline water from southern latitudes to Europe. In North Atlantic ocean the stream gives out a large amount of heat, cools down…

大气与海洋物理 · 物理学 2008-05-16 Ajay Patwardhan , Vivek Tewary

We present hemispherically resolved spectra of the surface of Europa from ~3.1--4.13 microns, which we obtained using the near infrared spectrometer NIRSPEC on the Keck II telescope. These include the first high-quality L-band spectra of…

地球与行星天体物理 · 物理学 2017-06-13 Samantha K. Trumbo , Michael E. Brown , Patrick D. Fischer , Kevin P. Hand

The tenuous atmospheres of the Galilean satellites are sourced from their surfaces and produced by a combination of plasma-surface interactions and thermal processes. Though thin, these atmospheres can be studied via their auroral…

地球与行星天体物理 · 物理学 2023-02-17 Katherine de Kleer , Zachariah Milby , Carl Schmidt , Maria Camarca , Michael E. Brown

Universal small-scale solar activity in quiet region are suggested to be a potential source of solar wind and the upper solar atmosphere. Here, with the high-resoltion 174 \AA~imaging observations from the Solar Orbiter/Extreme Ultraviolet…

太阳与恒星天体物理 · 物理学 2024-12-19 Yadan Duan , Hechao Chen , Zhenyong Hou , Zheng Sun , Yuandeng Shen

A weak absorption feature at 2.07 \textmu m on Europa's trailing hemisphere has been suggested to arise from radiolytic processing of an endogenic salt, possibly sourced from the interior ocean. However, if the genesis of this feature…

地球与行星天体物理 · 物理学 2023-08-29 M. Ryleigh Davis , Michael E. Brown , Samantha K. Trumbo

The composition of Europa's trailing hemisphere reflects the combined influences of endogenous geologic resurfacing and exogenous sulfur radiolysis. Using spatially resolved visible-wavelength spectra of Europa obtained with the Hubble…

地球与行星天体物理 · 物理学 2020-12-23 Samantha K. Trumbo , Michael E. Brown , Kevin P. Hand

Since the discovery of an ice particle plume erupting from the south polar terrain on Saturn's moon Enceladus, the geophysical mechanisms driving its activity have been the focus of substantial scientific research. The pattern and…

地球与行星天体物理 · 物理学 2018-10-10 Ben Southworth , Sascha Kempf , Joe Spitale

The New Horizons spacecraft has found evidence for geologic activity on the surface of Pluto, including extensional tectonic deformation of its water ice bedrock (see Moore et al., 2016). One mechanism that could drive extensional tectonic…

地球与行星天体物理 · 物理学 2016-08-03 Noah P. Hammond , Amy C. Barr , Edgar M. Parmentier

Europa's leading hemisphere chaos regions have a spectral feature at 450 nm that has been attributed to absorption by crystal defects in irradiated sodium chloride, known as F-centers. Some discrepancies exist between the laboratory data of…

地球与行星天体物理 · 物理学 2022-01-06 William T. P. Denman , Samantha K. Trumbo , Michael E. Brown

A link between exposures of water (H${}_{2}$O) ice with traces of an ammoniated compound (e.g., a salt) and the probable effusion of a water-rich cryolava onto the surface of Pluto has been established in previous investigations (Dalle Ore…

地球与行星天体物理 · 物理学 2023-06-28 A. Emran , C. M. Dalle Ore , D. P. Cruikshank , J. C. Cook

The outgassing signatures of Io, Europa, Enceladus, Triton, and Io-like exomoons are the focus of this review chapter. The rocky volcanic world of Io is unique in our Solar System, with plumes reaching to hundreds of kilometres in altitude.…

All numerical simulations of compressible convection reveal the presence of strong downwards directed flows. Thanks to helioseismology, such plumes have now been detected also at the top of the solar convection zone, on super- granular…

天体物理学 · 物理学 2015-06-24 Jean-Paul Zahn

We report on the shape dynamics of ice suspended in cold fresh water and subject to the natural convective flows generated during melting. Experiments reveal shape motifs for increasing far-field temperature: Sharp pinnacles directed…

流体动力学 · 物理学 2022-02-09 Scott Weady , Joshua Tong , Alexandra Zidovska , Leif Ristroph

The surface of Europa contains many quasi-circular morphologies called lenticulae. Although the formation mechanism of lenticulae is not understood, sill intrusion from the subsurface ocean is one promising hypothesis. However, it remains…

地球与行星天体物理 · 物理学 2018-10-16 Daigo Shoji

We perform a quantitative assessment for the potential for photosynthesis in hydrothermal vents in the deep ocean. The photosynthetically active radiation in this case is from geothermal origin: the infrared thermal radiation emitted by hot…

地球与行星天体物理 · 物理学 2015-06-15 Noel Perez , Rolando Cardenas , Osmel Martin , Michel Leiva-Mora