A blue band light curve for a flare of V1581 Cygni. The left-most point shows a 1 sigma error bar. Adapted from Cristaldi and Rodonò (1976) [1] | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
GJ 1245 AC | |
Right ascension | 19h 53m 55.142s [2] |
Declination | +44° 24′ 44.39″ [2] |
Apparent magnitude (V) | 13.46 / 16.75 [3] |
GJ 1245 B | |
Right ascension | 19h 53m 55.141s [4] |
Declination | +44° 24′ 54.15″ [4] |
Apparent magnitude (V) | 14.01 [3] |
Characteristics | |
Spectral type | M6V / M8V [5] / M6V [6] |
Variable type | UV Cet [7] |
Astrometry | |
Radial velocity (Rv) | 3.93±0.38 [4] km/s |
Proper motion (μ) | RA: 349.363(56) mas/yr [4] Dec.: −480.322(54) mas/yr [4] |
Parallax (π) | 214.5745 ± 0.0476 mas [4] |
Distance | 15.200 ± 0.003 ly (4.660 ± 0.001 pc) |
Absolute magnitude (MV) | 15.12 / 18.41 [5] / 15.72 [3] |
Orbit [8] | |
Primary | GJ 1245 A |
Companion | GJ 1245 C |
Period (P) | 6147±17 d |
Semi-major axis (a) | 0.8267±0.0008″ |
Eccentricity (e) | 0.334±0.002 |
Inclination (i) | 135.7±0.1° |
Longitude of the node (Ω) | 261.2±0.2° |
Periastron epoch (T) | 51506.8±2.1 |
Argument of periastron (ω) (secondary) | 36.1±0.2° |
Details | |
GJ 1245 A | |
Mass | 0.120±0.001 [5] M☉ |
Radius | 0.146±0.007 [5] R☉ |
Luminosity | 0.0014 [5] L☉ |
Temperature | 2,927 [5] K |
Metallicity [Fe/H] | -0.07 [5] dex |
Age | ~300[ citation needed ] Myr |
GJ 1245 C | |
Mass | 0.081±0.001 [5] M☉ |
Radius | 0.087±0.004 [5] R☉ |
Luminosity | 0.0003 [5] L☉ |
Temperature | 2,611 [5] K |
Metallicity [Fe/H] | -0.08 [5] dex |
Other designations | |
GJ 1245 AC: G 208-44, LHS 3494, NLTT 48414, KIC 8451868, 2MASS J19535443+4424541 [9] | |
GJ 1245 B: G 208-45, LHS 3495, NLTT 48415, KIC 8451881, 2MASS J19535508+4424550 [6] | |
Database references | |
SIMBAD | The system |
A | |
C | |
B | |
Location of GJ 1245 in the constellation Cygnus |
GJ 1245 (Gliese 1245) is a double star with components G 208-44 and G 208-45, located 15.2 light-years (4.7 parsecs ) away in the constellation Cygnus. G 208-44 is itself a closer double star made up of two red dwarfs, while G 208-45 is also a red dwarf. GJ 1245 is the 43rd closest stellar system to the Solar System. [10] GJ 1245 A and B are active flare stars, [11] and the pair are collectively designated V1581 Cygni. [12]
The largest of the three stars, GJ 1245 A (G 208-44 A) is only 12% the Sun's mass. [5] Of the other two stars, GJ 1245 C (G 208-44 B), is closest to star A at 2 AU away; [13] it is 8% of the Sun's mass. [5] The third star, GJ 1245 B (G 208-45), is 27 AU away from star A, [13] and is 10% of the Sun's mass; it would appear as bright as Venus does from Earth when viewed from star A.[ citation needed ]
TZ Arietis is a red dwarf in the northern constellation of Aries. With a normal apparent visual magnitude of 12.3, it is too faint to be seen by the naked eye, although it lies relatively close to the Sun at a distance of 14.6 light-years. It is a flare star, which means it can suddenly increase in brightness for short periods of time.
Gliese 674(GJ 674) is a small red dwarf star with an exoplanetary companion in the southern constellation of Ara. It is too faint to be visible to the naked eye, having an apparent visual magnitude of 9.38 and an absolute magnitude of 11.09. The system is located at a distance of 14.8 light-years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −2.9 km/s. It is a candidate member of the 200 million year old Castor stream of co-moving stars.
9 Aurigae is a star system in Auriga (constellation). It has an apparent magnitude of about 5, making it visible to the naked eye in many suburban skies. Parallax estimates made by the Hipparcos spacecraft put it at about 86 light-years from the solar system, although individual Gaia Data Release 3 parallaxes place all three components at 88 light years.
HD 40979 is a triple star system in the northern constellation of Auriga. The combined brightness of this group lies below the typical limit of visibility to the naked eye at an apparent visual magnitude of 6.74. It is located at a distance of approximately 108 light years from the Sun based on parallax. The system is receding with a radial velocity of +32 km/s. It has a relatively high rate of proper motion, traversing the celestial sphere at the rate of 0.182″ per year.
Gliese 412 is a pair of stars that share a common proper motion through space and are thought to form a binary star system. The pair have an angular separation of 31.4″ at a position angle of 126.1°. They are located 15.8 light-years distant from the Sun in the constellation Ursa Major. Both components are relatively dim red dwarf stars.
HD 178911 is a triple star system with an exoplanetary companion in the northern constellation of Lyra. With a combined apparent visual magnitude of 6.70, it is a challenge to view with the naked eye. The system is located at a distance of approximately 161 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −38 km/s.
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GJ 1062 is a single red dwarf star in the constellation Eridanus, positioned about two degrees to the SSE of Epsilon Eridani. It is also known as LHS 20 and Ross 578. The star is invisible to the naked eye with an apparent visual magnitude of +13.0, requiring a telescope with at least a 25 cm (10 in) aperture to view. It is located at a distance of 52.7 light years from the Sun based on parallax, but is drifting closer with a radial velocity of −85 km/s. The star has a high proper motion, traversing the sky at the rate of 3.033 arcseconds per year.
G 9-38, also known as EI Cancri and GJ 1116, is a binary star system consisting of two M-type stars. At 16.7 light-years from the Sun, the system is relatively nearby. The system has a very high stellar flare activity, with average five flares per hour.
Gliese 754 is a dim star in the southern constellation of Telescopium. It has an apparent visual magnitude of 12.25, which requires a telescope to view. The star is located at a distance of 19.3 light-years from the Sun based on parallax, and it is drifting further away with a radial velocity of +7 km/s. It is one of the hundred closest stars to the Solar System. Calculations of its orbit around the Milky Way showed that it is eccentric, and indicate that it might be a thick disk object.
ADS 7251 is a binary star system 6.33 parsecs from the Sun. The components are near-identical red dwarfs separated by 17″ in 2019.
EQ Pegasi is a nearby binary system of two red dwarfs. Both components are flare stars, with spectral types of M4Ve and M6Ve respectively, and a current separation between the components of 5.8 arcseconds. The system is at a distance of 20.4 light-years, and is 950 million years old. The primary star is orbited by one known exoplanet.
GJ 1128 is a red dwarf star of spectral type M4.0V, located in constellation Carina 21 light-years away from Earth. It is one of the closer stars to the Sun.
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HD 197037 is a binary star system. Its primary or visible star, HD 197037 A, is a F-type main-sequence star. Its surface temperature is 6150±34 K. HD 197037 A is depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.16±0.03, but is younger at an age of 3.408±0.924 billion years.
HD 155448 is a quintuple star system consisting of 5 young B-type stars. With an apparent magnitude of 8.72, it is too dim to be visible with the naked eye.
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