HD 31698
DSS image of HD 31698
Overlaid DSS image of HD 31698, 60' x 60' with north at top and west to the right

Aladin viewer for the region around HD 31698
Σ 622, BD+01 869, WDS J04581+0141, SAO 112275

Type  Binary Star
Magnitude  8.1
Right Ascension  4h 58' 6.2"  (2000)
Declination  1° 40' 32" N
Constellation  Orion
Description  Binary 8.4/8.6 2.6" 162°
Classification  F7V
Observing Notes

Andrew Cooper
Nov 26, 2022    Waikoloa, HI (map)
28cm f/10 SCT, NexStar 11" GyPSy @ 127x
Seeing: 6 Transparency: 7 Moon: 0%

A tight binary and a challenging split this morning, after recollimating the 'scope was able to achieve a clean split of two nearly equal magnitude stars separated by about 2" at a PA of 160 , 7' southwest of π6 Ori

Captain William Henry Smyth
Dec 2, 1833    No. 6 The Crescent, Bedford, England (map)
150mm f/17.6 refractor by Tully 1827

A fine double star, just preceding Orion's right knee; and at rather more than a third of the distance from Rigel to Aldebaran, where it is intersected by a line passed from Pollux through Bellatrix.

A 8½, white; B 9. pale grey. This exquisite object is 68 ♅ I.; and having had a retrograde angular motion of 0°.269 per annum assigned to it, was very carefully attended to. My measures, though they exhibit a slight change, do not countenance the amount mentioned; since, supposing ♅.'s to form a standard for its epoch, it would only be about 5° for upwards of half a century. Since this was discussed the great Dorpat Catalogue has arrived, by which a confirmation of other measures is obtained. The whole previous results are:
    ♅. Pos. 174°51'  Dist. 2".0±  Ep. 1782.85
S. 173°49' 2".56 1825.04
Σ. 179°54' 2".64 1832.09
[WDS 162° 2".60 2020
Smyth's estimate of 5° in 50 years (or 0.1°/yr) turns out to be
quite accurate when compared to 179° to 162° from 1832 to 2020]
― A Cycle of Celestial Objects Vol II, The Bedford Catalogue, William Henry Smyth, 1844
Other Data Sources for HD 31698
Nearby objects for HD 31698
Credits...

Drawings, descriptions, and CCD photos are copyright Andrew Cooper unless otherwise noted, no usage without permission.

A complete list of credits and sources can be found on the about page

HD 31698