17/05/2009, 17:55
18/05/2009, 12:17
18/05/2009, 20:50
Pinotti...................!Ufologo 555 ha scritto:
No, Danomars; e nemmeno tra i circa 500 casi di "fenomeni" lunari segnalati (più o meno ufficialmente), non li ho visti nemmen o sul volume scritto da Pinotti dove appunto li riporta; ma quelli che ho postao non li leggo da nessuna parte!
19/05/2009, 00:49
Enkidu ha scritto:
la prima, quella con l'anello azzurro, è davvero molto interessante.
Si può sapere dove si trova, e di cosa si tratta?
19/05/2009, 08:39
19/05/2009, 12:35
Biohazard ha scritto:
Il cratere si chiama Reiner e si trova nell'Oceanus Procellarum.
19/05/2009, 13:02
giancarlo selvatico ha scritto:Biohazard ha scritto:
Il cratere si chiama Reiner e si trova nell'Oceanus Procellarum.
Ma l'alone azzurro che lo circonda dovrebbe essere ghiaccio? o mi sbaglio
19/05/2009, 21:59
Thethirdeye ha scritto:
Auguriamocelo.....
19/05/2009, 22:05
giancarlo selvatico ha scritto:Biohazard ha scritto:
Il cratere si chiama Reiner e si trova nell'Oceanus Procellarum.
Ma l'alone azzurro che lo circonda dovrebbe essere ghiaccio? o mi sbaglio
19/05/2009, 22:22
Biohazard ha scritto:
Non si sa esattamente come si sia originato ma è un accumulo di materiali saliti in superficie.
20/05/2009, 12:06
The Clementine experiment carried four scientific imaging cameras: the Ultraviolet/Visible (UVVIS), Near-Infrared (NIR), High-Resolution (HiRES), and Long-wave Infrared (LWIR) cameras. The Ultraviolet/Visible (UVVIS) camera imaged the surface of the Moon at five wavelengths spanning the ultraviolet to near-infrared spectrum and the Near-Infrared (NIR) camera collected data at six wavelengths extending into the short-wave infrared (see tables below). This experiment yielded information on the color and inferred compositional properties of lunar soils and surface units, and also provided images useful for morphologic studies and cratering statistics. Most images were taken at low Sun angles, which is useful for compositional studies but not for observing morphology. Global mosaics at the five UVVIS and six NIR coregistered wavelengths were created using nearly 1 million images and are displayed here at a resolution of ~100 m/pixel.
In order to investigate the composition and origin of Reiner Gamma, near-infrared spectra and vidicon images were obtained and interpreted. The 0.40/0.56 micron ratio image shows that the high albedo portion of Reiner Gamma is surrounded by a 'red halo' and the 0.95/0.56 micron image indicates that Reiner Gamma exhibits a strong pyroxene absorption band. Analysis of the near-infrared spectra of various portions of the formation indicated the presence of major amounts of fresh mare basalt. Spectral mixing models demonstrate that the Reiner Gamma spectra can be reproduced by mixing major amounts of local fresh mare material (Reiner K crater) with small amounts of fresh highlands material (Oelbers A crater). No evidence was found for the presence of 'exotic' components (i.e., magnetite, free iron, cometary material). Together with photogeologic considerations, these results suggest that Reiner Gamma is quite young and is composed of a mixture of fresh highland materials with much larger quantities of local mare basalt.
What you are about to see will amaze you. It also should make you stop and think...
Why have they withheld these all these years...
Talk about cover-up... lets hear the excuses for this one...
20/05/2009, 15:37
20/05/2009, 17:53
20/05/2009, 18:11
20/05/2009, 19:12