HD 202206 b
Encyclopedia
HD 202206 b is a substellar object orbiting the star HD 202206
approximately 151 light-year
s away in the constellation
of Capricornus
. The classification of this object as an extrasolar planet
or a brown dwarf
is currently unclear. With a mass at least 17.4 times that of Jupiter
, it exceeds the limit (approximately 13 Jupiter masses) required for an object to sustain deuterium
fusion
in its core. The deuterium fusion criterion is used by the IAU
's Working Group on Extrasolar Planets to define the boundary between giant planets and brown dwarfs, so in this view HD 202206 b is a brown dwarf. On the other hand, simulations of planet formation by core accretion
show that objects of up to 25-30 Jupiter masses can be produced in this way, and therefore the object can potentially be regarded as a planet.
HD 202206
HD 202206 is a yellow dwarf star approximately 151 light-years away in the constellation Capricornus. The star is orbited by two companions with substellar masses in a near-resonant configuration.- Distance, age and metallicity :...
approximately 151 light-year
Light-year
A light-year, also light year or lightyear is a unit of length, equal to just under 10 trillion kilometres...
s away in the constellation
Constellation
In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....
of Capricornus
Capricornus
Capricornus is one of the constellations of the zodiac; it is often called Capricorn, especially when referring to the corresponding astrological sign. Its name is Latin for "horned male goat" or "goat horn", and it is commonly represented in the form of a sea-goat: a mythical creature that is half...
. The classification of this object as an extrasolar planet
Extrasolar planet
An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars...
or a brown dwarf
Brown dwarf
Brown dwarfs are sub-stellar objects which are too low in mass to sustain hydrogen-1 fusion reactions in their cores, which is characteristic of stars on the main sequence. Brown dwarfs have fully convective surfaces and interiors, with no chemical differentiation by depth...
is currently unclear. With a mass at least 17.4 times that of Jupiter
Jupiter
Jupiter is the fifth planet from the Sun and the largest planet within the Solar System. It is a gas giant with mass one-thousandth that of the Sun but is two and a half times the mass of all the other planets in our Solar System combined. Jupiter is classified as a gas giant along with Saturn,...
, it exceeds the limit (approximately 13 Jupiter masses) required for an object to sustain deuterium
Deuterium
Deuterium, also called heavy hydrogen, is one of two stable isotopes of hydrogen. It has a natural abundance in Earth's oceans of about one atom in of hydrogen . Deuterium accounts for approximately 0.0156% of all naturally occurring hydrogen in Earth's oceans, while the most common isotope ...
fusion
Nuclear fusion
Nuclear fusion is the process by which two or more atomic nuclei join together, or "fuse", to form a single heavier nucleus. This is usually accompanied by the release or absorption of large quantities of energy...
in its core. The deuterium fusion criterion is used by the IAU
IAU
IAU may refer to:*International Astronomical Union*International American University*International American University College of Medicine*International Association of Universities*International Association of Ultrarunners...
's Working Group on Extrasolar Planets to define the boundary between giant planets and brown dwarfs, so in this view HD 202206 b is a brown dwarf. On the other hand, simulations of planet formation by core accretion
Accretion (astrophysics)
In astrophysics, the term accretion is used for at least two distinct processes.The first and most common is the growth of a massive object by gravitationally attracting more matter, typically gaseous matter in an accretion disc. Accretion discs are common around smaller stars or stellar remnants...
show that objects of up to 25-30 Jupiter masses can be produced in this way, and therefore the object can potentially be regarded as a planet.