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  2. Interior Characterization of Europa using Magnetometry

    en.wikipedia.org/wiki/Interior_Characterization...

    Magnetic induction is a powerful tool for probing the subsurface and determine Europa's ocean depth, salinity, and ice shell thickness, as well as detecting erupting plume activity. The Principal Investigator is Carol Raymond, at NASA's Jet Propulsion Laboratory. [2]

  3. Weichselian glaciation - Wikipedia

    en.wikipedia.org/wiki/Weichselian_glaciation

    The Fennoscandian Ice Sheet of the Weichselian glaciation most likely grew out of a mountain glaciation of small ice fields and ice caps in the Scandinavian Mountains.The initial glaciation of the Scandinavian Mountains would have been enabled by moisture coming from the Atlantic Ocean and the mountains high altitude.

  4. Lake Vostok - Wikipedia

    en.wikipedia.org/wiki/Lake_Vostok

    Lake Vostok (Russian: озеро Восток, romanized: ozero Vostok) is the largest of Antarctica's 675 known [3] subglacial lakes.Lake Vostok is located at the southern Pole of Cold, beneath Russia's Vostok Station under the surface of the central East Antarctic Ice Sheet, which is at 3,488 m (11,444 ft) above mean sea level.

  5. Radar for Europa Assessment and Sounding: Ocean to Near ...

    en.wikipedia.org/wiki/Radar_for_Europa...

    The Radar for Europa Assessment and Sounding: Ocean to Near-surface (REASON) is a multi-frequency, multi-channel ice penetrating radar system that will be flown on board the Europa Clipper mission to Jupiter's moon Europa. REASON investigation will provide the first direct measurements of Europa's ice shell surface character and subsurface ...

  6. Europa (moon) - Wikipedia

    en.wikipedia.org/wiki/Europa_(moon)

    Europa was discovered independently by Simon Marius and Galileo Galilei [2] and was named (by Marius) after Europa, the Phoenician mother of King Minos of Crete and lover of Zeus (the Greek equivalent of the Roman god Jupiter). Slightly smaller than Earth's Moon, Europa is made of silicate rock and has a water-ice crust [16] and probably an ...

  7. European Project for Ice Coring in Antarctica - Wikipedia

    en.wikipedia.org/wiki/European_Project_for_Ice...

    End of the EDML ice core from a depth 2775 m; consists of meltwater which has formed at the basis of the ice sheet; the core was drilled 2002-2004 through the Antarctic ice sheet in the area of Dronning Maud Land by the project EPICA

  8. Tectonics on icy moons - Wikipedia

    en.wikipedia.org/wiki/Tectonics_on_Icy_Moons

    Europa's ice crust may be fractured by tidal stresses from Jupiter, and it has been hypothesized that liquid water could reach the surface through these cracks. [6] However, the ice overburden pressure within the crust exceeds tidal stresses at depths greater than 35 m below the ice surface, thereby limiting the depth at which tidally-induced ...

  9. Radioglaciology - Wikipedia

    en.wikipedia.org/wiki/Radioglaciology

    Radioglaciology is the study of glaciers, ice sheets, ice caps and icy moons using ice penetrating radar.It employs a geophysical method similar to ground-penetrating radar and typically operates at frequencies in the MF, HF, VHF and UHF portions of the radio spectrum.