If there is ammonia on Ceres that could mean
the dwarf planet formed in the outer part of the solar system, near Neptune.
«But it fits in perfectly with our understanding of how this remarkable
dwarf planet formed.»
The findings could help scientists better decipher the history of how
the dwarf planet formed, he added.
Not exact matches
Early images taken by New Horizons of the
dwarf planet's surface mean we have to rethink how the
planet was
formed
Now, to find out how the glaciers
formed in the first place, scientists created models that simulated atmospheric circulation on the
dwarf planet for the last 50,000 years (a mere 200 orbits around the sun for Pluto).
They soon realized the pair
formed when two
dwarf planets collided in the outer solar system.
An oversized free - floating
planet formed by agglomeration would not have a disk, explains Lada, so these
dwarfs must have
formed like stars.
It's hard to know how they
formed: The brown
dwarfs seem too heavy to have
formed from the slow agglomeration of material, like jumbo - sized
planets such as Jupiter.
Explaining an ammonia - rich Ceres may require either pushing the
dwarf planet's birthplace much farther out from the sun or importing showers of ammonia - rich pebbles from the outer solar system to help
form Ceres where it now resides.
Another 2016 study found that minerals called carbonates — which need water to
form — are spread across the
dwarf planet, suggesting that Ceres once hosted an ancient ocean.
Project Blue's proposed telescope would have a light - gathering mirror just half a meter wide — so small that it could only look for Earth - like
planets around two stars: the Sun - like Alpha Centauri A and Alpha Centauri B, which along with the red
dwarf Proxima Centauri
form the nearest star system to our own at just over four light - years away.
The proposed Phobos - Deimos
forming impactor would be between the size of the asteroid Vesta, which has a diameter of 326 miles, and the
dwarf planet Ceres, which is 587 miles wide.
There's an intriguing twist, too: Jayawardhana and others have shown that young brown
dwarfs generally do not have massive protoplanetary disks of gas and dust, which means that if the new object is indeed a
planet, it may not have
formed the same way
planets in our solar system did.
Mercedes Lopez - Morales, an astronomer at the Harvard - Smithsonian Center for Astrophysics, has modeled the possibilities of magnetic fields around red
dwarf planets, and a picture is gradually emerging: The
planets likely
form in the outer parts of their solar systems and migrate in.
How such a dense
planet formed is unclear, the researchers say, but it's probably the crystalline vestige of a white
dwarf star whose atmosphere was stripped away by the parent pulsar.
It's not yet clear how this binary system
formed, but the discovery may help redefine the line between
planets and brown
dwarfs — failed stars tens of times the mass of Jupiter.
Other astronomers find the detections convincing, although most reserve the name «
planet» for bodies that
form within a planetary system and orbit stars, says theorist Alan Boss of the Carnegie Institution of Washington in Washington, D.C. «They should call them «planetary - mass brown
dwarfs,»» Boss says.
Cartoon showing how efficient
planet migration around red
dwarfs lead to the more observed
planets than around sunlike stars, even though the disk is lower in mass and
forms fewer
planets in total.
We know that protoplanetary disks around red
dwarfs are lower in mass, so we expected them to
form fewer or smaller
planets.
- When brown
dwarfs were just a theoretical concern, astronomers differentiated those hypothetical objects from
planets by how they were
formed.
When heated by the distant sun, the materials are converted directly into vapors, which then fall back to the
dwarf planet in the
form of precipitation.
Researchers have long wondered if the little
dwarf planet could be the home for some
form of life.
The data gives researchers an understanding of how the
planet and its companion brown
dwarf formed, according to NASA.
Another
dwarf star, TRAPPIST - 1, with 8 % of the solar mass, was discovered recently3, 4 to host 3 habitable
planets out of a total of 7 and if life
forms in one of the three it will likely spread to the others5.
On the
dwarf planet, the reddish color is likely caused by tholins, which are
formed when cosmic rays and solar ultraviolet light interact with methane in Pluto's atmosphere and on its surface.
Astronomers have discovered direct evidence of water on the
dwarf planet Ceres in the
form of vapor plumes erupting into space, possibly from volcano - like ice geysers on its surface.
If
planets form around brown
dwarfs, then we have to add them to our list of possible abodes for life.
Moreover, the brown
dwarf companion to 15 Sge may eventually prove to have a highly circular orbit that is coplanar with the circumstellar disk so that
planets formed in inner orbits around the star.
Good news for them: a new study suggests that the
dwarf planet club could get another member, in the
form of a very small, distant object located roughly 92 astronomical units (AU) from the Sun.
The orbit of an Earth - like
planet around the tight binary system that star Ba
forms with its brown
dwarf companion in the liquid water zone would have to be centered around 1.1 AU — a little farther than Earth's orbital distance around Sol — with an orbital period exceeding one Earth year.
We don't know how you would
form these things,» she said, referring to
planets orbiting brown
dwarfs.
The brown
dwarf /
planet system is, in turn, orbiting around «A»,
forming a three - object system around 1,600 lightyears away from Earth.
That means that the
planet could have
formed from a ring of dust around the brown
dwarf, rather than the two objects
forming together as a sort of binary.
Some researchers even hold that
planets could
form around brown
dwarf and protoplanetary disks have already been found around a few of them.