Lacaille 9352
Encyclopedia
Lacaille 9352 is a red dwarf
star approximately 3.29 pc
or 10.74 light years from Earth's Solar System
. This star has the fourth highest known proper motion
, moving a total of 6.9 arcseconds per year. (This is still a very small movement overall, however, as there are 3,600 arcseconds in a degree of arc.) It is the tenth closest star system to the Solar System
and is the closest star in the constellation
Piscis Austrinus
. The ChView simulation shows that its closest neighbour is the EZ Aquarii
triple star system
at about 4.1 ly
from Lacaille 9352.
This was the first red dwarf star to have its angular diameter measured. The space velocity components of this star are = . If the radial velocity
(Vr) equals +9.7 km/s then about 2,700 years ago Lacaille 9352 was at its minimal distance of approximately 3.26 pc
from the Sun.
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 approximately 3.29 pc
Parsec
The parsec is a unit of length used in astronomy. It is about 3.26 light-years, or just under 31 trillion kilometres ....
or 10.74 light years from Earth's Solar System
Solar System
The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it, all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. The vast majority of the system's mass is in the Sun...
. This star has the fourth highest known proper motion
Proper motion
The proper motion of a star is its angular change in position over time as seen from the center of mass of the solar system. It is measured in seconds of arc per year, arcsec/yr, where 3600 arcseconds equal one degree. This contrasts with radial velocity, which is the time rate of change in...
, moving a total of 6.9 arcseconds per year. (This is still a very small movement overall, however, as there are 3,600 arcseconds in a degree of arc.) It is the tenth closest star system to the Solar System
Solar System
The Solar System consists of the Sun and the astronomical objects gravitationally bound in orbit around it, all of which formed from the collapse of a giant molecular cloud approximately 4.6 billion years ago. The vast majority of the system's mass is in the Sun...
and is the closest star 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....
Piscis Austrinus
Piscis Austrinus
Piscis Austrinus is a constellation in the southern celestial hemisphere. The name is Latin for "the southern fish" in contrast with the larger constellation Pisces, which represents a pair of fishes. Prior to the 20th century, it was also known as Piscis Notius...
. The ChView simulation shows that its closest neighbour is the EZ Aquarii
triple star system
EZ Aquarii
EZ Aquarii is a triple star system approximately from the Sun in the constellation Aquarius. It is also known as Luyten 789-6 and Gliese 866 and all three components are M-type red dwarfs. The pair EZ Aquarii AC form a spectroscopic binary with a 3.8 day orbit and a 0.03 AU separation. This...
at about 4.1 ly
Ly
Ly may refer to:* Ly the Fairy, a character from Rayman 2: The Great Escape* Lý Dynasty, a dynasty of Vietnam* Ly * Libya, ISO 3166-1 country code** .ly, the Top-level domain for Libya...
from Lacaille 9352.
This was the first red dwarf star to have its angular diameter measured. The space velocity components of this star are = . If the radial velocity
Radial velocity
Radial velocity is the velocity of an object in the direction of the line of sight . In astronomy, radial velocity most commonly refers to the spectroscopic radial velocity...
(Vr) equals +9.7 km/s then about 2,700 years ago Lacaille 9352 was at its minimal distance of approximately 3.26 pc
Parsec
The parsec is a unit of length used in astronomy. It is about 3.26 light-years, or just under 31 trillion kilometres ....
from the Sun.