This is a photo of the small island of Litla Dimun which is situated between Suouroy and Stora Dimun in the Faroe Islands. It is the smallest of the Islands being less than 100 hectares (250 acres) in size and it is uninhabited. The island is often covered by lenticular clouds. Lenticular clouds, also known as altocumular standing lenticularis clouds, are formed when a current of moist air is forced upwards as it travels over elevated land. This elevation and subsequent decrease in temperature causes the moisture in the air to condense and form a cloud. Lenticular clouds appear to be perfectly stationary but in fact this is not the case. These clouds only appear stationary because the flow of moist air continually resupplies the cloud from the windward side even as water evaporates and vanishes from the leeward side. Lenticular clouds can look like they are hovering for hours or days, until the wind or weather changes and the clouds disperse. They also look like a hat! -Jean Photo courtesy of Caters news agency.
Total solar eclipse, 2 July 2019.
Credits: ESA/CESAR
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Comet Hale-Bopp
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A dirty thunderstorm (also volcanic lightning, thunder volcano) is a weather phenomenon that is related to the production of lightning in a volcanic plume.
A study in the journal Science indicated that electrical charges are generated when rock fragments, ash, and ice particles in a volcanic plume collide and produce static charges, just as ice particles collide in regular thunderstorms.
Volcanic eruptions are sometimes accompanied by flashes of lightning. However, this lightning doesn’t descend from storm clouds in the sky. It is generated within the ash cloud spewing from the volcano, in a process called charge separation.
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Cassini mosaic of Iapetus, showing the bright trailing hemisphere with part of the dark area appearing on the right (the equatorial ridge is in profile on the right limb). The large crater Engelier is near the bottom; to its lower right can be seen the rim of a partly obliterated, slightly smaller older crater, Gerin.
This false-color mosaic shows the entire hemisphere of Iapetus (1,468 kilometers, or 912 miles across) visible from Cassini on the outbound leg of its encounter with the two-toned moon in Sept. 2007.
Credit: NASA/JPL
#cassini #iapetus #japeto #satellite #moon #lua #saturno #saturn #astronomy #astronomia https://www.instagram.com/p/B0kBRIHg3pQ/?igshid=meuno7r2ifg8
Known as the Horsehead Nebula – but you can call it Starbiscuit.
Found by our Hubble Space Telescope, this beauty is part of a much larger complex in the constellation Orion.
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The total solar eclipse of 02 July 2019 from La Serena, Chile.
Credit: Gwenael Blanck
Moons of Saturn Image Credit: Cassini Imaging Team, SSI, JPL, NASA
Explanation: On July 29, 2011 the Cassini spacecraft’s narrow-angle camera took this snapshot and captured 5 of Saturn’s moons, from just above the ringplane. Left to right are small moons Janus and Pandora respectively 179 and 81 kilometers across, shiny 504 kilometer diameter Enceladus, and Mimas, 396 kilometers across, seen just next to Rhea. Cut off by the right edge of the frame, Rhea is Saturn’s second largest moon at 1,528 kilometers across. So how many moons does Saturn have? Twenty new found outer satellites bring its total to 82 known moons, and since Jupiter’s moon total stands at 79, Saturn is the Solar System’s new moon king. The newly announced Saturnian satellites are all very small, 5 kilometers or so in diameter, and most are in retrograde orbits inclined to Saturn’s ringplane. You can help name Saturn’s new moons, but you should understand the rules. Hint: A knowledge of Norse, Inuit, and Gallic mythology will help.
∞ Source: apod.nasa.gov/apod/ap191017.html