Struve 1694
Σ 1694 A
|
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Camelopardalis |
Right ascension |
12h 49m 13.6s |
Declination |
+83° 24′ 46.4″ |
Apparent magnitude (V) |
5.28
|
Characteristics |
Spectral type |
A1IIIsh |
U−B color index |
-0.06 |
B−V color index |
-0.03 |
Astrometry |
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|
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Radial velocity (Rv) | 2.3 km/s | Proper motion (μ) | RA: -0.029 mas/yr Dec.: 0.020 mas/yr | Parallax (π) | 10.63 ± 1.74 mas | Distance | approx. 310 ly (approx. 90 pc) | Absolute magnitude (MV) | +0.54 | |
Details |
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|
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Rotation | 275 Km/s | |
Orbit |
Orbit |
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Companion | CCDM 12492+8325 B |
Other designations |
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HR 4893, HD 112028, BD+84°290, HIP 62572, SAO 2102, Σ 1694 A, STF 1694 A, Struve 1694 A, GC 17443, ADS 8682 A, CCDM 12492+8325 A. |
Database references |
---|
SIMBAD | data |
Data sources: |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
Database references |
---|
SIMBAD | data |
|
Σ 1694 B
|
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Camelopardalis |
Right ascension |
12h 49m 06.6s |
Declination |
+83° 25′ 04.2″ |
Apparent magnitude (V) |
5.85
|
Characteristics |
Spectral type |
A0V + A2V |
U−B color index |
-0.12 |
B−V color index |
-0.06 |
Astrometry |
---|
|
---|
Radial velocity (Rv) | 1 km/s | Proper motion (μ) | RA: -0.026 mas/yr Dec.: 0.022 mas/yr | Parallax (π) | 14.68 ± 6.92 mas | Distance | approx. 200 ly (approx. 70 pc) | |
Details |
---|
|
---|
Rotation | 17 Km/s | |
Orbit |
Orbit |
---|
Companion | CCDM 12492+8325 A |
Other designations |
---|
HR 4892, HD 112014, BD+84°289, HIP 62561, SAO 2101, Σ 1694 B, STF 1694 B, Struve 1694 B, GC 17440, ADS 8682 B, CCDM 12492+8325 B. |
Database references |
---|
SIMBAD | data |
Data sources: |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
Database references |
---|
SIMBAD | data |
|
Struve 1694 (Σ 1694, Struve 1694) is a star in the constellation Camelopardalis.[1]
Σ 1694 is a double star, with components of magnitudes 5.3m and 5.9m. Primary, Σ 1694 A is a white A-type subgiant with an apparent magnitude of 5.28m. It is approximately 300 light years from Earth. Secondary, Σ 1694 B is a spectroscopic binary both A-type main sequence star. Norton's Star Atlas describes the pair as yellowish and bluish.[1]
Σ 1694 was also known as 32H. Cam (Hevelius' 32nd of Camelopardalis), not Flamsteed's "32 Cam". Fl. 32 Cam is identical with 30 Aur. In British Association Catalogue, the star pair are belonging to the constellation Ursa Minor.
Chinese name
In Chinese, 北極 (Běi Jí), meaning North Pole, refers to an asterism consisting of Σ 1694, γ Ursae Minoris, β Ursae Minoris, 5 Ursae Minoris and 4 Ursae Minoris.[2] Consequently, Σ 1694 itself is known as 北極五 (Běi Jí wǔ, English: the Fifth Star of North Pole.),[3] representing 天樞 (Tiānshū), meaning Celestial Pivot.[4]
Notes