Ross 614 (V577 Monocerotis) is a
red dwarf UV Ceti
Luyten 726-8, also known as Gliese 65, is a binary star system that is one of Earth's nearest neighbors, at about 8.7 light years from Earth in the constellation Cetus. The two component stars are both flare stars with the variable st ...
flare star
A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes. It is believed that the flares on flare stars are analogous to solar flares in that they are due to the magnetic energy stored in th ...
and it is the primary member of a nearby
binary star system in the constellation of
Monoceros
Monoceros (Greek: Μονόκερως, "unicorn") is a faint constellation on the celestial equator. Its definition is attributed to the 17th-century Dutch cartographer Petrus Plancius. It is bordered by Orion to the west, Gemini to the north, ...
. This star has a
magnitude
Magnitude may refer to:
Mathematics
*Euclidean vector, a quantity defined by both its magnitude and its direction
*Magnitude (mathematics), the relative size of an object
*Norm (mathematics), a term for the size or length of a vector
*Order of ...
of about 11, making it invisible to the unaided eye even though it is one of the stars nearest to the Sun.
This system is among the closest to the
Sun
The Sun is the star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radi ...
at an estimated distance of about 13.3
light years. Because this star is so close to the Earth it is often the subject of study, hence the large number of designations by which it is known.
Binary star system
This binary star system consists of two closely spaced low-mass
red dwarfs. The secondary star is a dim
magnitude
Magnitude may refer to:
Mathematics
*Euclidean vector, a quantity defined by both its magnitude and its direction
*Magnitude (mathematics), the relative size of an object
*Norm (mathematics), a term for the size or length of a vector
*Order of ...
14 lost in the glare of the nearby primary star.
A study by
George Gatewood
George David Gatewood (born 1940) also known as ''George G. Gatewood'', is an American astronomer and presently is professor emeritus at the University of Pittsburgh and at the Allegheny Observatory. He specializes in astronomy, astronomical instru ...
in 2003 using older sources along with data from the
Hipparcos satellite yielded an orbital period of about 16.6 years and a semi-major axis separation of about 1.1 arc seconds (2.4–5.3 AU).
The most recent determination of the system orbital elements comes from a 2022 study combining data from
radial velocity,
astrometry, and imaging, which finds a similar orbital period, a
semi-major axis of 4.2 AU, and a very low mass for the companion of .
History
The primary star was discovered in 1927 by
F. E. Ross using the
refractor telescope
A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens (optics), lens as its objective (optics), objective to form an image (also referred to a dioptrics, dioptric telescope). The refracting telescope d ...
at the
Yerkes Observatory
Yerkes Observatory ( ) is an astronomical observatory located in Williams Bay, Wisconsin, United States. The observatory was operated by the University of Chicago Department of Astronomy and Astrophysics from its founding in 1897 to 2018. Owner ...
. He noticed the high
proper motion of this dim 11th magnitude star in his second-epoch plates that were part of an
astronomical survey
An astronomical survey is a general map or image of a region of the sky (or of the whole sky) that lacks a specific observational target. Alternatively, an astronomical survey may comprise a set of images, spectra, or other observations of ob ...
started by
E. E. Barnard, his predecessor at the observatory. Ross then included this new star in his eponymous catalog along with many others he discovered.
The first detection of a binary system was in 1936 by
Dirk Reuyl
Dirk Reuyl (1906 – 1972) was a Dutch people, Dutch United States, American physicist and astronomer. He was the cousin of astronomer Peter van de Kamp.
Life
Like his cousin, Reuijl (later "Reuyl") was born in Kampen, Overijssel. He studied p ...
using the 26-in
refractor telescope
A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens (optics), lens as its objective (optics), objective to form an image (also referred to a dioptrics, dioptric telescope). The refracting telescope d ...
of the
McCormick Observatory
The Leander McCormick Observatory is one of the astronomical observatories operated by the Department of Astronomy of the University of Virginia, and is situated just outside Charlottesville, Virginia (US) in Albemarle County on the summit of Mo ...
at the
University of Virginia
The University of Virginia (UVA) is a public research university in Charlottesville, Virginia. Founded in 1819 by Thomas Jefferson, the university is ranked among the top academic institutions in the United States, with highly selective ad ...
using
astrometric
Astrometry is a branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies. It provides the kinematics and physical origin of the Solar System and this galaxy, the Milky Way.
His ...
analysis of photographic plates. In 1951
Sarah L. Lippincott made the first reasonably accurate predictions of the position of the secondary star using the
refractor telescope
A refracting telescope (also called a refractor) is a type of optical telescope that uses a lens (optics), lens as its objective (optics), objective to form an image (also referred to a dioptrics, dioptric telescope). The refracting telescope d ...
of the
Sproul Observatory
Sproul Observatory was an astronomical observatory owned and operated by Swarthmore College. It was located in Swarthmore, Pennsylvania, United States, and named after William Cameron Sproul, the 27th Governor of Pennsylvania, who graduated ...
.
These calculations were used by
Walter Baade
Wilhelm Heinrich Walter Baade (March 24, 1893 – June 25, 1960) was a German astronomer who worked in the United States from 1931 to 1959.
Biography
The son of a teacher, Baade finished school in 1912. He then studied maths, physics and astr ...
to find and optically resolve this binary system for the first time using the then new
Hale Telescope
The Hale Telescope is a , 3.3 reflecting telescope at the Palomar Observatory in San Diego County, California, US, named after astronomer George Ellery Hale. With funding from the Rockefeller Foundation in 1928, he orchestrated the planning, de ...
at the
Palomar Observatory in
California
California is a state in the Western United States, located along the Pacific Coast. With nearly 39.2million residents across a total area of approximately , it is the most populous U.S. state and the 3rd largest by area. It is also the m ...
.
See also
*
List of nearest stars
This list covers all known stars, brown dwarfs, and sub-brown dwarfs within of the Sun. So far, 131 such objects have been found, of which only 22 are bright enough to be visible without a telescope. The visible light needs to reach or exce ...
References
Notes
{{DEFAULTSORT:Ross 614
Local Bubble
M-type main-sequence stars
Monoceros (constellation)
Binary stars
614
__NOTOC__
Year 614 ( DCXIV) was a common year starting on Tuesday (link will display the full calendar) of the Julian calendar. The denomination 614 for this year has been used since the early medieval period, when the Anno Domini calendar era ...
030920
0234
Monocerotis, V577