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| Risultati della ricerca nelle immagini - "Neruda" |
Grigna-2019-11-11_at_08_34_52.gifOne "Clear Day" to remember... (by Tatiana Balbiani in Fienga)163 visite"...Se saprai starmi vicino,
E potremo essere diversi,
Se il sole illuminer entrambi
Senza che le nostre ombre si sovrappongano,
Se riusciremo ad essere noi, in mezzo al mondo
E insieme al mondo, piangere, ridere, vivere.
Se ogni giorno sar scoprire quello che siamo
E non il ricordo di come eravamo,
Se sapremo darci l'un l'altro
Senza sapere chi sar il primo e chi l'ultimo
Se il tuo corpo canter con il mio perch insieme gioia...
Allora sar amore
E non sar stato vano aspettarsi tanto..."
(Pablo Neruda)MareKromium
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ZQ-Mercury-PIA10611.jpgNew Names for Features on Mercury54 visiteThe International Astronomical Union (IAU) recently approved new names for features on Mercury that were all seen for the first time in images taken by MESSENGER during the Spacecraft's first flyby of the Planet.
Read the full press release for additional details about the naming process and the origin of the names, and visit the U.S.G.S. website, the Gazetteer of Planetary Nomenclature, to learn about all of the named planetary features in the Solar System.
This image, produced by mosaicking many Narrow Angle Camera (NAC) images together, shows the locations of the newly named features, along with the craters Basho, Mozart, and Tolstoj, first seen by the Mariner 10 Mission.
Close-up views of many of these features are available in the MESSENGER website image gallery. In particular, look at these previous releases for NAC high-resolution images of Apollodorus, Beagle Rupes, Eminescu, Mozart, Neruda, Pantheon Fossae, Raditladi and Sander.MareKromium
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ZZ-Mercury-Craters-Atget_Crater-PIA10934.jpgAtget Crater (natural colors; credits: Lunexit)53 visiteRecently named for the French photographer Eugne Atget, Atget Crater, seen in the middle of the lower portion of this NAC image, is distinctive on Mercury's Surface due to its dark color. Atget Crater is located within Caloris Basin, near Apollodorus Crater and Pantheon Fossae, which are also both visible in this image to the North-West of Atget. The dark color of the floor of Atget is in contrast to other craters within Caloris Basin that exhibit bright materials on their floors, such as the craters Kertsz and Sander. Other craters on Mercury, such as Basho and Neruda, have halos of dark material but the dark material does not cover the crater floors. Understanding the variety of bright and dark materials associated with different craters will provide insight into Mercury's composition and the processes that acted on Mercury's Surface.
Date Acquired: January 14, 2008
Image Mission Elapsed Time (MET: 108828540
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Resolution: 520 meters/pixel (0,32 miles/pixel)
Scale: This image shows a scene about 530 Km (approx. 330 miles) across
Spacecraft Altitude: about 20.300 Km (approx. 12.600 miles)MareKromium
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ZZ-Mercury-Craters-Neruda_Crater-PIA17515-PCF-LXTT-IPF-0.jpgNeruda Crater (CTX Frame - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)68 visiteThis frame features the Mercurian Impact Crater named "Neruda", after the Chilean poet Pablo Neruda (born on July, 12, 1904 in Parral - Chile - and died on September, 23, 1973 in the Chilean State's Capital, Santiago). As you can see, this Impact Crater (whose diameter is approx. 112 Km - such as about 69,55 miles) exhibits several Central Peaks punctuated by a few more recent, small Craters, resulting in a rugged Surface mostly made of ups and downs (and now think how difficult it would be if one hypothetical Astronaut decided - or just needed - to traverse the whole Crater's highly irregular Floor...). Similarly, the Crater's namesake Pablo Neruda experienced a number of ups and downs in his life, from success as a poet, through poverty, war and ultimately alleged poisoning.
Date acquired: July, 24th, 2012
Image Mission Elapsed Time (MET): 251577944
Image ID: 2256593
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 52,20 South
Center Longitude: 125,30 East
Solar Incidence Angle: 80,4 (meaning that the Sun, at the time that the picture was taken, was about 9,6 above the imaged Local Mercurian Horizon)
Emission Angle: 2,4
Sun-Mercury-Messenger (or "Phase") Angle: 78,0
This picture (which is an Original NASA - MESSENGER Spacecraft's b/w and Map-Projected image published on the NASA - Planetary Photojournal with the ID n. PIA 17515) has been additionally processed, contrast enhanced, magnified and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - MESSENGER Spacecraft and then looked down, towards the Surface of Mercury), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team. Different colors, as well as different shades of the same color, mean, among other things, the existence of different Elements (Minerals) present on the Surface of Mercury, each having a different Albedo (---> Reflectivity) and Chemical Composition.MareKromium
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ZZ-Mercury-Craters-Neruda_Crater-PIA17515-PCF-LXTT-IPF-1.jpgNeruda Crater (EDM - Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga/Lunar Explorer Italia/Italian Planetary Foundation)69 visiteThis frame is an Extra Detail Magnification (or "EDM", for short) featuring the Central Peaks' System of the Mercurian Impact Crater named "Neruda", after the Chilean poet Pablo Neruda (born on July, 12, 1904 in Parral - Chile - and died on September, 23, 1973 in the Chilean State's Capital, Santiago). As you can see, this Impact Crater (whose diameter is approx. 112 Km - such as about 69,55 miles) exhibits several Central Peaks punctuated by a few more recent, small Craters, resulting in a rugged Surface mostly made of ups and downs (and now think how difficult it would be if one hypothetical Astronaut decided - or just needed - to traverse the whole Crater's highly irregular Floor...). Similarly, the Crater's namesake Pablo Neruda experienced a number of ups and downs in his life, from success as a poet, through poverty, war and ultimately alleged poisoning.
Date acquired: July, 24th, 2012
Image Mission Elapsed Time (MET): 251577944
Image ID: 2256593
Instrument: Narrow Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 52,20 South
Center Longitude: 125,30 East
Solar Incidence Angle: 80,4 (meaning that the Sun, at the time that the picture was taken, was about 9,6 above the imaged Local Mercurian Horizon)
Emission Angle: 2,4
Sun-Mercury-Messenger (or "Phase") Angle: 78,0
This picture (which is a crop taken from an Original NASA - MESSENGER Spacecraft's b/w and Map-Projected image published on the NASA - Planetary Photojournal with the ID n. PIA 17515) has been additionally processed, contrast enhanced, magnified to aid the visibility of the details and then colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - MESSENGER Spacecraft and then looked down, towards the Surface of Mercury), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team. Different colors, as well as different shades of the same color, mean, among other things, the existence of different Elements (Minerals) present on the Surface of Mercury, each having a different Albedo (---> Reflectivity) and Chemical Composition.MareKromium
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ZZ-Mercury-Limb-PIA16820-PCF-LXTT-IPF.jpgSouthern Craters (Absolute Natural Colors; credits for the additional process. and color.: Dr Paolo C. Fienga - Lunar Explorer Italia/Italian Planetary Foundation)73 visiteThe set of 3 (three) frames shown here in Absolute Natural Colors and forming this image mosaic, was acquired by the NASA - MESSENGER Spacecraft as part of a sequence intended to monitor any changes in the calibration of the Multispectral Wide Angle Camera onboard the Spacecraft over time. However, the final result of this "calibration" also gives us a simply beautiful view of a wide portion (the whole scene is approx. 1900 Km - such as a little less of 1180 miles - across) of Mercury's heavily cratered Southern Hemisphere. Furthermore, the Impact Craters Magritte, Neruda, and Sher-Gil can be easily spotted within this scene. North is towards the top-left of the image.
Date acquired: December, 17th, 2012
Images Mission Elapsed Time (MET): 264237810, 264237814, 264237830
Images ID: 3157538, 3157539, 3157543
Instrument: Wide Angle Camera (WAC) of the Mercury Dual Imaging System (MDIS)
Center Latitude: 59,16 South
Center Longitude: 149,3 East
Resolution: 1663 meters/pixel
Solar Incidence Angle: 59,2 (meaning that the Sun, at the time that the pictures were taken, was about 30,8 above the imaged Local Mercurian Horizon)
Emission Angle: 28,8
Sun-Mercury-Messenger (or "Phase") Angle: 78,1
This picture (which is an Original NASA - MESSENGER Spacecraft color image mosaic published on the NASA - Planetary Photojournal with the ID n. PIA 16820) has been additionally processed and then re-colorized in Absolute Natural Colors (such as the colors that a human eye would actually perceive if someone were onboard the NASA - MESSENGER Spacecraft and then looked outside, towards the Surface of Mercury), by using an original technique created - and, in time, dramatically improved - by the Lunar Explorer Italia Team. Different colors, as well as different shades of the same color, mean, among other things, the existence of different Elements (Minerals) present on the Surface of Mercury, each having a different Albedo (---> Reflectivity) and Chemical Composition.MareKromium
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