HD 74389
Double star system in the constellation Ursa Major
From Wikipedia, the free encyclopedia
HD 74389 is a double star system approximately 425 light years from Earth. The primary, HD 74389 A, was initially listed in the Hipparcos catalog as an A0V spectral type star, but this was subsequently updated in 1990 as A2V when Sanduleak and Pesch imaged it with the Burrell Schmidt telescope at Kitt Peak.[10]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Ursa Major[1] |
| HD 74389 A | |
| Right ascension | 08h 45m 46.92304s[2] |
| Declination | +48° 52′ 43.5507″[2] |
| Apparent magnitude (V) | 7.48[3] |
| HD 74389 B | |
| Right ascension | 08h 45m 46.92304s[4] |
| Declination | +48° 52′ 43.5507″[4] |
| Apparent magnitude (V) | 14.62[3] |
| Characteristics | |
| Spectral type | A2V + DA1.3 + M?[3] |
| U−B color index | +0.05[5] |
| B−V color index | +0.07[5] |
| Astrometry | |
| HD 74389 A | |
| Radial velocity (Rv) | −15.4[6] km/s |
| Proper motion (μ) | RA: −2.097±0.096[2] mas/yr Dec.: 8.067±0.076[2] mas/yr |
| Parallax (π) | 7.6401±0.0633 mas[2] |
| Distance | 427 ± 4 ly (131 ± 1 pc) |
| Absolute magnitude (MV) | 1.2[3] |
| HD 74389 B | |
| Proper motion (μ) | RA: −1.437±0.089[4] mas/yr Dec.: 7.605±0.075[4] mas/yr |
| Parallax (π) | 7.6689±0.0729 mas[4] |
| Distance | 425 ± 4 ly (130 ± 1 pc) |
| Absolute magnitude (MV) | 9.4[3] |
| Orbit[7] | |
| Period (P) | 80,000 yr |
| Semi-major axis (a) | 2488.5 AU |
| Details | |
| A | |
| Mass | 1.71[7] M☉ |
| Luminosity | 9.71[8] L☉ |
| Temperature | 8.200[8] K |
| B | |
| Mass | 0.69[7] M☉ |
| Radius | 0.015[3] R☉ |
| Luminosity | 0.4[3] L☉ |
| Surface gravity (log g) | 7.85[3] cgs |
| Temperature | 39,500[7] K |
| Other designations | |
| BD+49°1766, HIP 42994, TYC 3420-1971-1, GSC 03420-01971, 2MASS J08454693+4852435[9] | |
| Database references | |
| SIMBAD | data |
The primary component is a white A-type main sequence star with an apparent magnitude of +7.48. Its furthest companion, HD 74389 B, is a DA-type white dwarf located 20.11 arcseconds west of—at least 190 AU from—HD 74389 A, and has a V magnitude of 14.62.
On August 4, 2016, NASA's Goddard Space Flight Center announced that its citizen science program, Disk Detective, discovered a debris disk orbiting the primary, making this the first disk ever discovered around a star with a companion white dwarf.[11] Cataloged as DDOI AWI00000wz, the disk temperature was observed to be at most 136 K. Although stars with white dwarf companions are common, and there are three known planetary systems with white dwarfs as distant companions (Gl 86, HD 27442, and HD 147513), no debris disks had previously been discovered with a closely associated white dwarf.[12]