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  2. Mars sol - Wikipedia

    en.wikipedia.org/wiki/Mars_sol

    It is approximately 24 hours, 39 minutes, 35 seconds long. A Martian year is approximately 668.6 sols, equivalent to approximately 687 Earth days [ 1 ] or 1.88 Earth years. The sol was adopted in 1976 during the Viking Lander missions and is a measure of time mainly used by NASA when, for example, scheduling the use of a Mars rover .

  3. Timekeeping on Mars - Wikipedia

    en.wikipedia.org/wiki/Timekeeping_on_Mars

    The actual landing site was 0.900778° (19.8 km) east of that, corresponding to 3 minutes and 36 seconds later in local solar time. The date is kept using a mission clock sol count with the landing occurring on Sol 0, corresponding to MSD 47776 (mission time zone); the landing occurred around 16:35 LMST, which is MSD 47777 01:02 AMT.

  4. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Its surface contains a mixture of carbon, [148] frozen water and hydrated minerals. [149] There are signs of past cryovolcanic activity, where volatile material such as water are erupted onto the surface, as seen in surface bright spots. [150] Ceres has a very thin water vapor atmosphere, but practically speaking it is indistinguishable from a ...

  5. Water vapor - Wikipedia

    en.wikipedia.org/wiki/Water_vapor

    Water vapor can also be indirect evidence supporting the presence of extraterrestrial liquid water in the case of some planetary mass objects. Water vapor, which reacts to temperature changes, is referred to as a 'feedback', because it amplifies the effect of forces that initially cause the warming. Therefore, it is a greenhouse gas. [2]

  6. Sol (colloid) - Wikipedia

    en.wikipedia.org/wiki/Sol_(colloid)

    A sol is a colloidal suspension made out of tiny solid particles [1] in a continuous liquid medium. Sols are stable, so that they do not settle down when left undisturbed, and exhibit the Tyndall effect, which is the scattering of light by the particles in the colloid. The size of the particles can vary from 1 nm - 100 nm.

  7. Volatile (astrogeology) - Wikipedia

    en.wikipedia.org/wiki/Volatile_(astrogeology)

    In igneous petrology the term more specifically refers to the volatile components of magma (mostly water vapor and carbon dioxide) that affect the appearance and explosivity of volcanoes. Volatiles in a magma with a high viscosity , generally felsic with a higher silica (SiO 2 ) content, tend to produce eruptions that are explosive eruption .

  8. Planetary habitability in the Solar System - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability_in...

    This suspicion is caused because of the unusually high level of water vapor in the thin atmosphere of Ganymede. The moon likely has several layers of ice and liquid water, and finally a liquid layer in contact with the mantle. The core, the likely cause of Ganymede's magnetic field, would have a temperature near 1600 K.

  9. Vapor–liquid equilibrium - Wikipedia

    en.wikipedia.org/wiki/Vaporliquid_equilibrium

    In thermodynamics and chemical engineering, the vaporliquid equilibrium (VLE) describes the distribution of a chemical species between the vapor phase and a liquid phase. The concentration of a vapor in contact with its liquid, especially at equilibrium , is often expressed in terms of vapor pressure , which will be a partial pressure (a ...