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originally posted by: nonspecific
are you not plaugurising yourself?
originally posted by: Justshrug
Not to be too pedantic but shouldn't this be under Space Exploration
Also, anyone know if Ceres is ever viewable using amateur telescopes (I assume its too dark?)
originally posted by: Roxxo
Back on topic:
If the bright spots are geysers/ice volcanoes, what is the process behind them? The Jovian and Saturnian moons that have geysers and/or ice volcanoes have them because tidal forces squeeze and pull on the moon causing the inside to heat up. There isn't anything close enough to Ceres to do that and aren't small bodies like Ceres usually geologically dead?
originally posted by: Baltazar84
first off im not sure if this is the correct forum. if not feel free to move it
p.s. how the heck do you attach a photo?? i clicked insert an image and couldnt navigate anywhere..anyways heres the story
found it very interesting. as well as their "theories" on whats causing it. not sure if im buying the "its ice reflecting light" excuse
what do you guys think this could be??
originally posted by: Justshrug
Not to be too pedantic but shouldn't this be under Space Exploration
Also, anyone know if Ceres is ever viewable using amateur telescopes (I assume its too dark?)
originally posted by: w810i
I'm guessing right about the time it slips into orbit some sort of "Major" news will break here on earth that will shift focus away from this until it slips all the way out of the mainstream media.
originally posted by: w810i
I'm guessing right about the time it slips into orbit some sort of "Major" news will break here on earth that will shift focus away from this until it slips all the way out of the mainstream media.
2 Views of Ceres on Approach, Uncropped NASA's Dawn spacecraft obtained these uncropped images of dwarf planet Ceres on Feb. 19, 2015, from a distance of about 29,000 miles (46,000 kilometers). They are part of a series taken as Dawn observed Ceres completing one full rotation, which lasted about nine hours. The images show the full range of different crater shapes that can be found at Ceres' surface: From shallow, flattish craters to those with peaks at their centers. These views show sections of Ceres' surface that are similar to those in PIA19056 .