HR 4796
Encyclopedia
HR 4796 is a binary star system
approximately 220 light-year
s away in the constellation
of Centaurus. The system includes an A-type main sequence star
and a red dwarf
star. The primary star is twice as massive as the Sun and twenty times more luminous. It is thought to be approximately 8 million years old and is surrounded by a protoplanetary disk
that was discovered in 1991. The dust in the disk appears to be the result of collisions between planetesimal
s.
In 2007 observations using the Near-Infrared Multi-Object Spectrometer aboard the Hubble Space Telescope
indicated that the dust had a reddish spectrum similar to that of tholin
s.
Binary star
A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary...
approximately 220 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 Centaurus. The system includes an A-type main sequence star
Star
A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...
and a red dwarf
Red dwarf
According to the Hertzsprung-Russell diagram, a red dwarf star is a small and relatively cool star, of the main sequence, either late K or M spectral type....
star. The primary star is twice as massive as the Sun and twenty times more luminous. It is thought to be approximately 8 million years old and is surrounded by a protoplanetary disk
Protoplanetary disk
A protoplanetary disk is a rotating circumstellar disk of dense gas surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star...
that was discovered in 1991. The dust in the disk appears to be the result of collisions between planetesimal
Planetesimal
Planetesimals are solid objects thought to exist in protoplanetary disks and in debris disks.A widely accepted theory of planet formation, the so-called planetesimal hypothesis of Viktor Safronov, states that planets form out of cosmic dust grains that collide and stick to form larger and larger...
s.
In 2007 observations using the Near-Infrared Multi-Object Spectrometer aboard the Hubble Space Telescope
Hubble Space Telescope
The Hubble Space Telescope is a space telescope that was carried into orbit by a Space Shuttle in 1990 and remains in operation. A 2.4 meter aperture telescope in low Earth orbit, Hubble's four main instruments observe in the near ultraviolet, visible, and near infrared...
indicated that the dust had a reddish spectrum similar to that of tholin
Tholin
Tholin [after the ancient Greek word meaning "not clear"] is a heteropolymer molecule formed by solar ultraviolet irradiation of simple organic compounds such as methane or ethane. Tholins do not form naturally on modern-day Earth, but are found in great abundance on the surface of icy bodies in...
s.