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A little interesting about space life.
In a mysterious region beyond the orbit of the beautiful, banded, blue ice-giant planet Neptune--the most distant of the eight major planets from our Sun--there is a dark and frigid domain called the Kuiper Belt. Within this remote region, where our Sun shines with only a weak fire, and appears to be merely a particularly large star suspended in the black sky, a multitude of strange, icy worldlets tumble around our Star. Pluto, a large icy denizen inhabiting the Kuiper Belt, was originally classified as the ninth major planet from our Sun after its discovery in 1930. However, with the realization that this frozen "oddball" is really only one of several large, icy inhabitants of the Kuiper Belt, the International Astronomical Union (IAU) found it necessary to formally define "planet" in 2006--and poor Pluto was unceremoniously ousted from the pantheon of major planets. Pluto, now freshly reclassified as a dwarf planet, nonetheless remains a small world of great interest, debate, and affection. Scientists will soon learn much more about this beloved, distant, ice-ball so far away, when, after a treacherous nine-year journey of three million miles through interplanetary space, NASA's hearty New Horizons spacecraft arrives at Pluto on July 14, 2015.
and here is another
Pluto itself is a relatively large denizen of the distant Kuiper Belt, that orbits our Sun in the frigid company of a vast multitude of other bewitching and mysterious icy objects. Like other Kuiper Belt Objects (KBOs), Pluto is thought to be composed primarily of ice and rock. It is an intriguing frozen "oddball", a mere 1/6 the mass of Earth's own Moon and 1/3 its volume. Pluto also has a highly inclined, eccentric orbit that carries it from 30 to 49 Astronomical Units (AU) from our Sun. One AU is equal to the mean Earth-Sun separation of 93,000,000 miles. As a result, Pluto periodically moves towards our Sun at a distance that is closer to our Star than Neptune. Very fortunately for both Neptune and Pluto, an orbital resonance with Neptune prevents the duo from crashing into each other.
However, the fact of the matter is that moon will always remain the best option for mankind. The reason for this stems from the fact that the moon can always act as a stepping stone to the rest of the solar system and beyond. This is only natural, as the moon is in a very close proximity to Earth. Only by taking a 3 day trip, it is possible to reach the Moon with standard chemical propulsion techniques. However, in retrospect, going to Mars would require almost 100 times the amount of trip time of moon, since Mars is about 1000 times further then the moon. The amount of life support that is required for a mission that will take 2 years or more is definitely very costly and more importantly, the technological capability is not there. Thus, with our present global financial and technical capability, the moon is the only realistic option.
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For this reason, for many years astronomers considered the possibility that hydrocarbon lakes and seas might exist on this fantastic moon-world. Data that finally arrived courtesy of the joint NASA and European Space Agency's (ESA's) Cassini-Huygens mission lived up to their expectations. Since arriving at the Saturn system in 2004, the Cassini spacecraft has revealed more than 620,000 square miles of Titan's long-hidden, bewildering surface--and it has shown that almost two percent of Titan's entire surface is covered in liquid.
Titan is the largest moon of the gas-giant planet Saturn, as well as the second-largest moon in our entire Solar System--after Jupiter's enormous Ganymede. Indeed, this smoggy orange moon is almost as big as the planet Mars! Because Titan is situated in the outer domain of our Solar System, circling Saturn--which is the sixth major planet from our Star, the Sun--it is extremely cold, and its chemical atmosphere is frozen. This very interesting atmosphere is composed of a mix of compounds that many astronomers think are comparable to those that existed in our own planet's primordial atmosphere. Titan's strange, dense, orange atmosphere contains large quantities of "smoggy" hydrocarbons. This very heavy shroud of obscuring smog is so extremely dense that it showers "gasoline-like" rain down on the tortured surface of this distant moon-world.
"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.