Nebula Tutorial nebula tutorial by jkelly26 on deviantart Tutorial Nebula

Nebula Tutorial nebula tutorial by jkelly26 on deviantart Tutorial Nebula

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A little interesting about space life.

Multiple Light Sources. On the moon, there is only one light source sufficiently strong to form shadows; the Sun. So it is solid to suggest that all shadows on the Moon should run parallel to each other. However, this was apparently not the case during the moon landing.



and here is another

Like Earth's own large Moon, Triton is locked in synchronous rotation with its planet--one side always faces Neptune. However, because of Neptune's odd orbital inclination, both of the moon's polar regions take turns facing the Sun. Spacecraft images of Triton reveal mounds and round pits formed from icy lava flows (cryovolanism), as well as smooth volcanic plains. The surface of the moon is only sparsely cratered, indicating that its surface is new--that is, it is constantly being resurfaced, probably by the "lava" flow from icy volcanoes. Triton is very bright--its fresh, sparkling, new ice-coating is believed to cover a heart of metal and rock. Triton's high density suggests that it contains more rock in its interior than the icy moons of Saturn and Uranus.



and finally

Titan's alien climate--including its heavy hydrocarbon rain and fierce winds--forms surface features that are similar to those on Earth, and it experiences seasonal weather changes--just like our own planet. In fact, with its liquids pooling both on its surface and beneath its surface, along with its mostly nitrogen atmosphere, Titan has a methane cycle that is comparable to Earth's water cycle--although at the much more frosty temperature of about -179.2 degrees Celsius.

More information:

"This is still very much an area of active research, so there is much that scientists including our Department of Terrestrial Magnetism staff scientist Erik Hauri, as well as many other Carnegie colleagues and alumni, are figuring out about how much water exists on the Moon. This is a highly important and challenging question to answer given that we have limited knowledge on the history and distribution of lunar water," explained Dr. Miki Nakajima in a February 26, 2018 Carnegie Institution Press Release. Dr. Nakajima, who is of the Carnegie Institution of Washington (D.C.), along with California Institute of Technology's (Caltech's) Dr. David Stevenson, set out to determine whether prevailing lunar formation models need to be adjusted to explain more recent higher estimates of the quantity of water on Earth's Moon. Caltech is in Pasadena.



There are ongoing studies assessing the past habitability potential of the Red Planet, as well as the possibility of life.



"Our model explains the diversity of these ice-rich moons and the evidence for their very active geology and dynamics. It also explains a puzzling fact about Titan, in that a giant impact would give it a high orbital eccentricity," Asphaug continued to explain to the press on October 18, 2012.