| Piú viste - Asteroids and Comets |
Dart-2.jpgGreat Balls of Fire! - 270 visitenessun commentoMareKromium
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IDA&DACTYL-PIA00333.jpgIda and Dactyl in "natural colors"69 visiteThis color picture is made from images taken by the imaging system on the Galileo spacecraft about 14 minutes before its closest approach to asteroid 243 Ida on August 28, 1993. The range from the spacecraft was about 10,500 kilometers (6,500 miles). The images used are from the sequence in which Ida's moon was originally discovered; the moon is visible to the right of the asteroid. This picture is made from images through the 4100-angstrom (violet), 7560 A (infrared) and 9680 A (infrared) filters. The color is 'enhanced' in the sense that the CCD camera is sensitive to near infrared wavelengths of light beyond human vision; a 'natural' color picture of this asteroid would appear mostly gray. Shadings in the image indicate changes in illumination angle on the many steep slopes of this irregular body as well as subtle color variations due to differences in the physical state and composition of the soil (regolith).
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Comets-Comet_Hartley_2-EB-LXTT4.jpgComet "Hartley 2" (credits for the additional process. and color.: Elisabetta Bonora - Lunexit Team)69 visitenessun commentoMareKromium
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ZZ-ZZ-ZZ-ZZ-ZZ-ZZ-ZZ-ZZ-Ultima_Thule_2-flyby.gifUltima Thule (Fly-By)69 visiteOriginal Caption:"Mission scientists created this "departure movie" from 14 different images taken by the New Horizons Long Range Reconnaissance Imager (LORRI) shortly after the spacecraft flew past the Kuiper Belt object nicknamed Ultima Thule (officially named 2014 MU69) on Jan. 1, 2019".MareKromium
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Asteroids_from_HST-00.jpgAsteroids, from HST (1)68 visiteCaption NASA originale da "NASA - Picture of the Day" del 18 Aprile 2005:"Rocks from space hit Earth every day. The larger the rock, though, the less often Earth is struck. Many kilograms of space dust pitter to Earth daily. Larger bits appear initially as a bright meteor. Baseball-sized rocks and ice-balls streak through our atmosphere daily, most evaporating quickly to nothing. Significant threats do exist for rocks near 100 meters in diameter, which strike the Earth roughly every 1000 years. An object this size could cause significant tsunamis were it to strike an ocean, potentially devastating even distant shores. A collision with a Massive asteroid, over 1 Km across, is more rare, occurring typically millions of years apart, but could have truly global consequences".
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Lutetia-01.jpgAsteroid "Lutetia"68 visiteAsteroid Lutetia will no longer remain a mystery as the European Space Agency's (ESA) Rosetta has captured the first close-up images of this Celestial Body, which will help them gain insights into the composition of the space rock that has long puzzled the scientists.
In what can be termed as the closest encounter with one of the largest asteroid, ever visited ESA led robotic spacecraft mission, Rosetta, raced past Lutetia as close as 3200 Km, with the closest encounter at 18:10 CEST (Central Europe Standard Time), when the spacecraft was just 3162 Km away from the giant asteroid.
Rosetta, which had a first look of Lutetia in January 2007, has this time “triumphed at asteroid” and captured images like never before.MareKromium
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IDA-PIA00138.jpgAsteroid Ida's limb (HR)67 visiteThe Galileo imaging system captured this picture of the limb of the asteroid 243 Ida about 46 seconds after its closest approach on August 28, 1993, from a range of only 2480 Km. It is the highest-resolution image of an asteroid's surface ever captured and shows detail at a scale of about 25 meters per pixel. This image is one frame of a mosaic of 15 frames shuttered near Galileo's closest approach to Ida. Since the exact location of Ida in space was not well-known prior to the Galileo flyby, this mosaic was estimated to have only about a 50 percent chance of capturing Ida. Fortunately, this single frame did successfully image a part of the sunlit side of Ida. The area seen in this frame shows some of the same territory seen in a slightly lower resolution full disk mosaic of Ida returned from the spacecraft in September, 1993, but from a different perspective. Prominent in this view is a 2 Km deep "valley" seen in profile on the limb.
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Comets-Comet_Ikeya_Zhang_4.jpgComet Ikeya-Zhang - the "ion tail"67 visiteAs Comet Ikeya-Zhang approached the Sun, it developed a complex blue "ion tail". The "ion tail" is composed of ions that boiled off the nucleus and were pushed away from the Sun by the out-flowing fast-moving particles of the solar wind. Complexity in the tail is created by comet nucleus rotation, variability in the comet surface evaporation rate and variability of the Sun's magnetic field and solar wind.
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Tempel1-Z-I-HST.jpgThe impact sequence from HST67 visiteDa "NASA - Picture of the Day", del giorno 18 Luglio 2005:"It was a human-made event visible across the Solar System. At the direction of terrestrial scientists, a refrigerator-sized probe from the Deep Impact mission struck Comet Tempel-1 on July 4 at over 35.000 Km per hour.
The unexpectedly bright explosion was not nuclear but rather originated from a large plume that reflected back sunlight. Pictured above is how the event looked to the Earth-orbiting HST. A large cloud of bright material is seen emanating from the comet's nucleus and then dispersing. The area encompassing the comet became over two times brighter in the hours after the impact. Astronomers will continue to study the images and data returned by Deep Impact to better determine the nature of Comet Tempel-1 and discern clues about the formation dynamics of the early Solar System".
Nota: leggendo questa poche righe non serve uno Scienziato per capire che, al momento, l'unico scopo chiaro dell'esperimento era quello di fare propaganda...
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Comets-Comet_Holmes-0.jpgA "Light Arrow" is heading towards "Heart & Soul"...67 visiteCaption NASA:"Two spectacular comets graced Earth's skies during 2007.
Both comets became bright enough to be seen by the unaided eye of the casual sky enthusiast. Early in 2007, Comet McNaught grew brighter than any comet in 40 years, displaying a beautiful dust tail that flowed across the sky.
Comet McNaught (a.k.a. c/2006 P1) became known as the "Great Comet" of 2007, sported unusual striations in its expansive dust tail, and showed unexpectedly complex chemistry in its ion tail.
Toward the year's end, normally docile and faint Comet Holmes brightened suddenly and unexpectedly to naked eye visibility. Remarkably, Comet 17P/Holmes stayed bright for weeks even though it lies beyond the orbit of Mars.
No distant comet in recent history has remained so bright for so long.
In this view, a white Comet Holmes was photographed in early December posing with the Heart and Soul Nebulae".MareKromium
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Tempel1-ZZ-ZJ-Stardust_1024-MF-LXTT-HD3D.jpgComet Tempel-1 from Stardust NeXT Spacecraft (Hi-Def-3D; credits for the additional process.: Dr Marco Faccin - Lunexit Team)67 visitenessun commentoMareKromium
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EROS-PIA03129.jpgEros from above (2)66 visiteNEAR Shoemaker photographed this area of Eros on December 18, 2000, from an orbital altitude of 33 Km. This part of the asteroid's surface, like many others, appears vaguely "sculptured" due to its low, elongated ridges and depressions with seemingly consistent orientations. Some of the low spots also contain accumulations of smooth, pond-like materials. Neither the surface sculpturing nor the pond-like materials are well understood, and both will be investigated in detail using even higher-resolution images from NEAR Shoemaker's low passes over Eros in early 2001. The whole scene is about 1 Km across.
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