«Surprisingly, the host galaxy [of FRB 121102] is a puny, star -
forming dwarf system,» says ASTRON's Cees Bassa, who led the optical observations together with Shriharsh Tendulkar of McGill University in Montreal, Canada.
Not exact matches
They soon realized the pair
formed when two
dwarf planets collided in the outer solar
system.
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.
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.
«Asteroid ripped apart to
form star's glowing ring
system: Research includes first image of ring
system orbiting a white
dwarf.»
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.
Scholz's star is actually a binary
system formed by a small red
dwarf, with about 9 % of the mass of the Sun, around which a much less bright and smaller brown
dwarf orbits.
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.
If there is ammonia on Ceres that could mean the
dwarf planet
formed in the outer part of the solar
system, near Neptune.
There is another Barium -
dwarf candidate star, Chi1 Orionis or HR 2047 (G0 V), in the same Ursa Major stellar moving group, which suggests that all three stars may have
formed a multiple
system until their orbital stability was disrupted when the once, brighter and bigger AGB star shed most of an estimated original mass of 2.6 Solar to reveal its white
dwarf core about 30 million years ago (Porto de Mello and da Silva, 1997).
This hypothesis suggests that all three stars may have
formed a multiple
system until their orbital stability was disrupted when the once, brighter and bigger AGB star (HR 6094 B) shed most of an estimated original mass of 2.6 Solar to reveal its white
dwarf core about 30 million years ago (Porto de Mello and da Silva, 1997).
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.
The brown
dwarf / planet
system is, in turn, orbiting around «A»,
forming a three - object
system around 1,600 lightyears away from Earth.