Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Caelum |
Right ascension | 05h 01m 34.5225s [1] |
Declination | −39° 43′ 04.9641″ [1] |
Apparent magnitude (V) | 6.01±0.01 [2] |
Characteristics | |
Spectral type | G8 III [3] |
B−V color index | +0.88 [4] |
Astrometry | |
Radial velocity (Rv) | 5.73±0.12 [1] km/s |
Proper motion (μ) | RA: −5.456 [1] mas/yr Dec.: +32.717 [1] mas/yr |
Parallax (π) | 8.0168 ± 0.0344 mas [1] |
Distance | 407 ± 2 ly (124.7 ± 0.5 pc) |
Absolute magnitude (MV) | +0.78 [5] |
Details | |
Mass | 2.40 [6] M☉ |
Radius | 10.03 [7] [8] R☉ |
Luminosity | 50.1 [9] L☉ |
Surface gravity (log g) | 3.18±0.14 [10] cgs |
Temperature | 5,032±61 [9] K |
Metallicity [Fe/H] | −0.02±0.13 [10] dex |
Rotational velocity (v sin i) | 2±1.4 [11] km/s |
Age | 700 [6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 32453 (HR 1631) is a solitary star located in the southern constellation Caelum. With an apparent magnitude of 6.01, [2] it's barely visible to the naked eye under ideal conditions. This star is located 407 light years away based on its parallax shift, but is drifting away at a rate of 5.73 km/s. [1]
HD 32453 has a classification of G8 III, [3] which states it is an evolved G-type star that exhausted hydrogen at its core and left the main sequence. At present it has 2.40 [6] times the Sun's mass, but at an age of 700 million years, [6] HD 32453 has expanded to 10 [7] times the latter's girth (radius detected from an angular diameter of 0.748 mas [8] ). It radiates at 50 [9] solar luminosities from its enlarged photosphere at an effective temperature of 5,032 K, [9] which gives it a yellow hue. HD 32453 is slightly metal deficient, [10] and spins slowly with a projected rotational velocity of 2 km/s, [11] common for a giant star.
θ Trianguli Australis, Latinized as Theta Trianguli Australis, is a single star in the southern constellation of Triangulum Australe. It is visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of +5.50. The star is located about 334 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +10 km/s.
Omega Andromedae is the Bayer designation for a slowly co-rotating binary star system in the northern constellation of Andromeda. Parallax measurements made during the Gaia mission make this system to be approximately 93.9 light-years from Earth. Its apparent visual magnitude is +4.83, which makes it bright enough to be seen with the naked eye.
3 Aquarii is a variable star in the equatorial constellation of Aquarius. 3 Aquarii is the Flamsteed designation; it also bears the Bayer designation k Aquarii and the variable star designation EN Aquarii. With a mean apparent visual magnitude of 4.429, it is visible to the naked eye in dark skies. It has an annual parallax shift of 5.57 milliarcseconds with a 5% margin of error, which translates to a physical distance of around 590 light-years from Earth.
Tau Puppis, Latinized from τ Puppis, is a star in the southern constellation of Puppis, near the southern constellation boundary with Carina. It is visible to the naked with an apparent visual magnitude of +2.95 and is located at a distance of about 182 light-years from Earth. The variable radial velocity of this system was detected by H. D. Curtis and H. K. Palmer in 1908, based on observations made at the D. O. Mills Observatory. It is a spectroscopic binary star system, with the presence of the secondary component being revealed by the shifts of absorption lines in the spectrum resulting from the Doppler effect. The two components orbit each other with a period of 1,066.0 days and a low eccentricity of 0.090.
HD 197036 is a single star in the northern constellation Cygnus. It has an absolute magnitude of −1.15 and an apparent magnitude of 6.61, below the max naked eye visibility. Located 1,310 light years away, it is approaching Earth with a heliocentric radial velocity of −15 km/s.
HD 88809 is a star located in the southern constellation Antlia. With an apparent magnitude of 5.89 it is barely visible to the naked eye under ideal conditions. The star is located at a distance of around 451 light years but is drifting away at a heliocentric radial velocity of almost 20 km/s.
HD 200661 is a solitary star in the equatorial constellation Equuleus. It has an apparent magnitude of 6.41, placing it near the max naked eye visibility. The star is situated at a distance of 430 light years but is approaching with a heliocentric radial velocity of −12.1 km/s.
HD 10550 is a single star in the equatorial constellation of Cetus. It is a faint star but visible to the naked eye with an apparent visual magnitude of 4.98. Based upon an annual parallax shift of 2.9564 mas, it is located around 1,100 light years from the Sun. The star is moving closer with a heliocentric radial velocity of −33 km/s. It has a high peculiar velocity of 72.7+5.7
−4.3 km/s and may be a runaway star.
HD 74772 is a single star in the southern constellation of Vela. It is positioned near the Vela SNR, which gives it an intense X-ray background. The star is of apparent visual magnitude 4.05, and hence is visible to the naked eye. Based upon an annual parallax shift of 15.8 mas, it is located 207 light years from the Sun. It is moving closer to the Earth with a heliocentric radial velocity of −2 km/s.
GZ Velorum is a single, orange-hued star in the southern constellation of Vela. It is a faint star but visible to the naked eye, having an apparent visual magnitude of 4.58. The star is located around 1,300 light years from Earth, as determined from its annual parallax shift of 2.4 mas. It is moving further away with a heliocentric radial velocity of +13 km/s.
HD 89998 is a single star in the southern constellation of Vela. It is a faint star but visible to the naked eye with an apparent visual magnitude of 4.82. The distance to HD 89998, as determined from its annual parallax shift of 15.9 mas, is 205 light years. The star is moving further from the Earth with a heliocentric radial velocity of +21 km/s, having come within 140 ly some 1.552 million years ago.
3 Piscis Austrini, also known as HD 201901 or simply 3 PsA, is an astrometric binary located in the southern constellation Microscopium. It was once part of Piscis Austrinus, the southern fish. The system has a combined apparent magnitude of 5.39, making it faintly visible to the naked eye under ideal conditions. Gaia DR3 parallax measurements imply a distance of 404 light years and it is currently approaching the Solar System with a heliocentric radial velocity of −46.2 km/s. At its current distance, 3 PsA's brightness is diminished by 0.12 magnitudes due to extinction from interstellar dust and it has an absolute magnitude of +0.19.
HD 50002 is a solitary star in the southern circumpolar constellation Volans. It is faintly visible to the naked eye with an apparent magnitude of 6.09 and is located at a distance of 708 light years. However, it is drifting further with a heliocentric radial velocity of 5.1 km/s.
HD 55151 is a solitary star located in the circumpolar constellation Volans. With an apparent magnitude of 6.47, it is near the limit of naked eye visibility. The star is located 512 light years away from the Solar System, but is drifting closer with a heliocentric radial velocity of -13 km/s.
HD 166006, also known as HR 6778, is a solitary orange-hued star located in the southern constellation Telescopium. It has an apparent magnitude of 6.07, making it barely visible to the naked eye. Based on Gaia DR2 parallax measurements, the object is located 582 light years away. It is currently approaching the Solar System with a somewhat constrained heliocentric radial velocity of −15 km/s.
Iota Octantis, Latinized, from ι Octantis is a double star in the southern circumpolar constellation Octans. The "A" component has an apparent magnitude of 5.83, making it faintly visible to the naked eye under ideal conditions, but the "B" component can't be seen due to its faintness. The system is located at a distance of 350 light years based on its annual parallax shift, but is drifting away at a rate of 53.4 km/s.
HD 30479 is a solitary star in the southern circumpolar constellation Mensa. It has an apparent magnitude of 6.04, making it barely visible to the naked eye even under ideal conditions. It is located at a distance of 540 light years but is receding with a heliocentric radial velocity of 10.3 km/s.
HD 196775 is a solitary star in the equatorial constellation Delphinus. It has an apparent magnitude of 5.98, allowing it to be faintly seen with the naked eye. The object is relatively far at a distance of 1,050 light years but is approaching the Solar System with a heliocentric radial velocity of −4.6 km/s. HD 196775 has a high peculiar velocity of 21.8+1.9
−4.1 km/s compared to neighboring stars, indicating that it may be a runaway star.
HD 204018, also designated as HR 8202, is a visual binary located in the southern constellation Microscopium. The primary has an apparent magnitude of 5.58, making it faintly visible to the naked eye under ideal conditions. The companion has an apparent magnitude of 8.09. The system is located relatively close at a distance of 176 light years based on Gaia DR3 parallax measurements but is receding with a heliocentric radial velocity of 18.3 km/s. At its current distance, HD 204018's combined brightness is diminished by 0.13 magnitudes due to interstellar dust.
HD 25274, also known as HR 1241, is a solitary star located in the northern circumpolar constellation Camelopardalis. It is faintly visible to the naked eye as a red hued point of light with an apparent magnitude of 5.86. Gaia DR3 parallax measurements imply a distance of 597 light-years and it is currently drifting closer with a heliocentric radial velocity of −48.23 km/s. At its current distance, HD 25274's brightness is diminished by three-tenths of a magnitude due to interstellar extinction and it has an absolute magnitude of −0.51.