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  2. Atmosphere of Uranus - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Uranus

    Temperature profile of the Uranian troposphere and lower stratosphere. Cloud and haze layers are also indicated. The Uranian atmosphere can be divided into three main layers: the troposphere, between altitudes of −300 [a] and 50 km and pressures from 100 to 0.1 bar; the stratosphere, spanning altitudes between 50 and 4000 km and pressures between 0.1 and 10 −10 bar; and the thermosphere ...

  3. Climate of Uranus - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Uranus

    The variation of the microwave emission from Uranus is probably caused by changes in the deep tropospheric circulation, because thick polar clouds and haze may inhibit convection. [ 19 ] For a short period in the second half of 2004, a number of large clouds appeared in the Uranian atmosphere, giving it a Neptune -like appearance.

  4. Uranus - Wikipedia

    en.wikipedia.org/wiki/Uranus

    The lowest temperature recorded in Uranus's tropopause is 49 K (−224.2 °C; −371.5 °F), making Uranus the coldest planet in the Solar System. [ 18 ] [ 95 ] One of the hypotheses for this discrepancy suggests the Earth-sized impactor theorised to be behind Uranus's axial tilt left the planet with a depleted core temperature, as the impact ...

  5. Extraterrestrial atmosphere - Wikipedia

    en.wikipedia.org/wiki/Extraterrestrial_atmosphere

    The thin atmosphere also increases the variability of the planet's temperature. Martian surface temperatures vary from lows of approximately −140 °C (−220 °F) during the polar winters to highs of up to 20 °C (70 °F) in summers. The tenuous atmosphere of Mars visible on the horizon. Pits in south polar ice cap, MGS 1999, NASA

  6. Uranus’ mysterious features on display in new Webb image - AOL

    www.aol.com/news/uranus-hidden-rings-unusual...

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  7. Outline of Uranus - Wikipedia

    en.wikipedia.org/wiki/Outline_of_Uranus

    It is the coldest planetary atmosphere in the Solar System, with a minimum temperature of 49 K (−224.2 °C), and has a complex, layered cloud structure with water thought to make up the lowest clouds and methane the uppermost layer of clouds. The interior of Uranus is mainly composed of ice and rock.

  8. Microwave Sounding Unit temperature measurements - Wikipedia

    en.wikipedia.org/wiki/Microwave_Sounding_Unit...

    Once the orbital changes had been allowed for the data showed a 0.07K per decade increase in temperature at this level of the atmosphere. Another important critique of the early satellite record was its shortness—adding a few years on to the record or picking a particular time frame could change the trends considerably.

  9. Sudarsky's gas giant classification - Wikipedia

    en.wikipedia.org/wiki/Sudarsky's_gas_giant...

    For the very hottest gas giants, with temperatures above 1400 K (2100 °F, 1100 °C) or cooler planets with lower gravity than Jupiter, the silicate and iron cloud decks are predicted to lie high up in the atmosphere. The predicted Bond albedo of a class V planet around a Sun-like star is 0.55, due to reflection by the cloud decks.