| Risultati della ricerca nelle immagini - "Thermal" |
APOLLO_14_AS_14-77-10361a.JPGAS 14-77-10361 (a) - Thermal Degradation Sample58 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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APOLLO_14_AS_14-77-10362a.JPGAS 14-77-10362 (a) - Thermal Degradation Sample57 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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APOLLO_14_AS_14-77-10364a.JPGAS 14-77-10364 (a) - Thermal Degradation Sample63 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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APOLLO_14_AS_14-77-10365a.JPGAS 14-77-10365 (a) - Thermal Degradation Sample60 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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APOLLO_14_AS_14-77-10366a.JPGAS 14-77-10366 (a) - Thermal Degradation Sample58 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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APOLLO_14_AS_14-77-10367_HR-a.JPGAS 14-77-10367 (a) - Thermal Degradation Sample59 visiteThermal Degradation Sample; taken in the vicinity of Station "A".MareKromium
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PHOE-SOL099-PIA11073.jpgPhoenix Conductivity Probe after Extraction - Sol 99 (natural colors; credits: NASA)81 visiteCaption NASA:"NASA's Phoenix Mars Lander inserted the 4 needles of its Thermal and Conductivity Probe into Martian soil during the 98th Sol of the mission and left it in place until Sol 99 (Sept. 4, 2008).
The Surface Stereo Imager on Phoenix took this image on the morning of Sol 99 after the probe was lifted away from the soil. This imaging served as a check of whether soil had stuck to the needles.
The Thermal and Conductivity Probe measures how fast heat and electricity move from one needle to an adjacent one through the soil or air between the needles. Conductivity readings can be indicators about water vapor, water ice and liquid water.
The probe is part of Phoenix's Microscopy, Electrochemistry and Conductivity suite of instruments".MareKromium
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Thermal_Map-ORB410_01_surf_comp_H1.jpgThermal Map of Venusian Surface (comparison ESA/NASA)54 visiteCaption ESA:"An unprocessed thermal map of the Venusian Surface obtained by VIRTIS on 5 June 2007 (left) is compared here with a radar image of the same area obtained by NASA’s Magellan Spacecraft in the 1990s (right).
VIRTIS, the imaging spectrometer on board Venus Express, obtained this image at 1 micrometre, a wavelength that allows detection of radiation originating from the surface. The imaged region is that which NASA’s MESSENGER flew over as it made its closest approach to the Planet.
Magellan’s radar imaging and altimetry maps made it possible to measure the elevation and the radio-optical properties of the surface. Venus Express’ VIRTIS is providing the first complete set of thermal maps of the surface of Venus.
Correlations between topographic and thermal data similar to the ones shown in this image-composite will allow the scientists to understand if the measured temperature of the surface depends only on the altitude – where higher altitudes simply corresponds to colder, temperatures such as on Earth – or if it depends on the presence of previously undetected sources of heat such as active volcanoes".MareKromium
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