![]() A visual band light curve for LQ Hydrae. The main plot (adapted from Berdyugina et al. [1]) shows the long-term variation, and the inset plot (adapted from Kiraga [2]) shows the periodic variation. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 32m 25.568s [3] |
Declination | −11° 11′ 04.69″ [3] |
Apparent magnitude (V) | 7.82 [4] (7.79 to 7.86) [5] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | K1Vp [6] |
B−V color index | 0.933±0.021 [4] |
Variable type | BY Dra [5] |
Astrometry | |
Radial velocity (Rv) | 7.58±0.27 [7] km/s |
Proper motion (μ) |
RA: −248.040
mas/
yr
[3] Dec.: 34.277 mas/ yr [3] |
Parallax (π) | 54.7362 ± 0.0244 mas [3] |
Distance | 59.59 ± 0.03
ly (18.269 ± 0.008 pc) |
Absolute magnitude (MV) | 6.47 [6] |
Details | |
Mass | 0.81 [8] M☉ |
Radius | 1.0 [9] R☉ |
Luminosity | 0.282±0.001 [3] L☉ |
Surface gravity (log g) | 4.57 [8] cgs |
Temperature | 4,812±39 [8] K |
Metallicity [Fe/H] | 0.32 [8] dex |
Rotation | 1.601 [9] d |
Rotational velocity (v sin i) | 25±2 [10] km/s |
Age | Under 75 [11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
LQ Hydrae is a single [13] variable star in the equatorial constellation of Hydra. It is sometimes identified as Gl 355 from the Gliese Catalogue; LQ Hydrae is the variable star designation, which is abbreviated LQ Hya. [14] The brightness of the star ranges from an apparent visual magnitude of 7.79 down to 7.86, [5] which is too faint to be readily visible to the naked eye. Based on parallax measurements, this star is located at a distance of 59.6 light years from the Sun. It is drifting further away with a radial velocity of 7.6 km/s. [7]
During a 1981 survey of southern stars, W. P. Bidelman found the H and K lines of ionized calcium for LQ Hya were filled in with emission. ( W. D. Heintz independently made the same observation.) In 1986, F. C. Fekel and associates determined this is a young, rapidly rotating BY Draconis-type variable. [13] [15] A decade of photometry was used to determine a rotation period of 1.601136±0.000013 days (1 day, 14 hours, and 24 minutes) The star spots on the surface showed significant evolution over time scales of a few months. Variations in rotational modulation of surface activity suggested the star is undergoing differential rotation. [10]
The high lithium abundance and rapid rotation of this star indicate it is a zero age main sequence star, or possibly even a pre-main sequence star. [14] A strong flare event was observed on December 22, 1993, with an estimated energy release of ~5.7×1033 erg. [11] Additional flares were detected thereafter, with ROSAT X-ray data from 1992 showing a strong flare during that time period. [14] Observations from December 2000 and 2001 showed that the magnetic field of the star is dramatically changing its topology on a time frame of a year or less. [16]
The stellar classification of LQ Hya is K1Vp, [6] indicating it is a K-type main-sequence star with some peculiar features in the spectrum. In some respects it is considered an analog of a young Sun around the age of 60 million years. [1] It shows strong emission of ultraviolet and has been detected in the X-ray band, showing an X-ray emission of 8.8×1029 erg/s and indicating high chromospheric activity levels. [14] The star shows dual magnetic activity cycles with period of 6.8 and 11.4 years, [14] which are somewhat comparable to the solar cycle in the Sun.
![]() A visual band light curve for LQ Hydrae. The main plot (adapted from Berdyugina et al. [1]) shows the long-term variation, and the inset plot (adapted from Kiraga [2]) shows the periodic variation. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 32m 25.568s [3] |
Declination | −11° 11′ 04.69″ [3] |
Apparent magnitude (V) | 7.82 [4] (7.79 to 7.86) [5] |
Characteristics | |
Evolutionary stage | Main sequence |
Spectral type | K1Vp [6] |
B−V color index | 0.933±0.021 [4] |
Variable type | BY Dra [5] |
Astrometry | |
Radial velocity (Rv) | 7.58±0.27 [7] km/s |
Proper motion (μ) |
RA: −248.040
mas/
yr
[3] Dec.: 34.277 mas/ yr [3] |
Parallax (π) | 54.7362 ± 0.0244 mas [3] |
Distance | 59.59 ± 0.03
ly (18.269 ± 0.008 pc) |
Absolute magnitude (MV) | 6.47 [6] |
Details | |
Mass | 0.81 [8] M☉ |
Radius | 1.0 [9] R☉ |
Luminosity | 0.282±0.001 [3] L☉ |
Surface gravity (log g) | 4.57 [8] cgs |
Temperature | 4,812±39 [8] K |
Metallicity [Fe/H] | 0.32 [8] dex |
Rotation | 1.601 [9] d |
Rotational velocity (v sin i) | 25±2 [10] km/s |
Age | Under 75 [11] Myr |
Other designations | |
Database references | |
SIMBAD | data |
LQ Hydrae is a single [13] variable star in the equatorial constellation of Hydra. It is sometimes identified as Gl 355 from the Gliese Catalogue; LQ Hydrae is the variable star designation, which is abbreviated LQ Hya. [14] The brightness of the star ranges from an apparent visual magnitude of 7.79 down to 7.86, [5] which is too faint to be readily visible to the naked eye. Based on parallax measurements, this star is located at a distance of 59.6 light years from the Sun. It is drifting further away with a radial velocity of 7.6 km/s. [7]
During a 1981 survey of southern stars, W. P. Bidelman found the H and K lines of ionized calcium for LQ Hya were filled in with emission. ( W. D. Heintz independently made the same observation.) In 1986, F. C. Fekel and associates determined this is a young, rapidly rotating BY Draconis-type variable. [13] [15] A decade of photometry was used to determine a rotation period of 1.601136±0.000013 days (1 day, 14 hours, and 24 minutes) The star spots on the surface showed significant evolution over time scales of a few months. Variations in rotational modulation of surface activity suggested the star is undergoing differential rotation. [10]
The high lithium abundance and rapid rotation of this star indicate it is a zero age main sequence star, or possibly even a pre-main sequence star. [14] A strong flare event was observed on December 22, 1993, with an estimated energy release of ~5.7×1033 erg. [11] Additional flares were detected thereafter, with ROSAT X-ray data from 1992 showing a strong flare during that time period. [14] Observations from December 2000 and 2001 showed that the magnetic field of the star is dramatically changing its topology on a time frame of a year or less. [16]
The stellar classification of LQ Hya is K1Vp, [6] indicating it is a K-type main-sequence star with some peculiar features in the spectrum. In some respects it is considered an analog of a young Sun around the age of 60 million years. [1] It shows strong emission of ultraviolet and has been detected in the X-ray band, showing an X-ray emission of 8.8×1029 erg/s and indicating high chromospheric activity levels. [14] The star shows dual magnetic activity cycles with period of 6.8 and 11.4 years, [14] which are somewhat comparable to the solar cycle in the Sun.