The sky around vdB 92 at true scale, north up and east left, with stars to magnitude 8. The circles show the field of a low-power eyepiece and of 10×50 binoculars.
vdB 92 is a reflection nebula in Canis Major, 3,730 light-years away
vdB 92 is a reflection nebula in the constellation Canis Major, 3,730 light-years away. spans 8′ of sky, about 8.7 light-years across. It is a telescope object, 6 inches or larger, and it is highest in the evening sky in February.
Nebula: a cloud of gas and dust. Emission nebulae glow on their own, lit by ultraviolet light from hot young stars; reflection nebulae shine by starlight scattered from dust; dark nebulae block the light behind them.
vdB 92 is vdB 92 in the Van den Bergh catalog of reflection nebulae
Sidney van den Bergh listed it in his catalog of reflection nebulae (1966), drawn from the Palomar Sky Survey. He chose nebulae lit by a star bright enough to appear in the Bonner and Cordoba star catalogs. The star that lights it is BD-11 1763, magnitude 8.9. He rated it very faint in brightness and intermediate (uncertain) in color.
Finding vdB 92 from Sirius
vdB 92 lies 6.9° northeast of Sirius, the magnitude -1.4 star. Three fingers held at arm's length cover about 5°.
vdB 92 is highest in the evening in February
The chart gives its height above the horizon at 9 pm through the year, from 60°N to 40°S. It can be seen from the whole southern hemisphere and north to about 78°N, and never sets south of 78°S.
vdB 92 is 3,730 light-years away
The light seen from vdB 92 tonight left it about 3,730 years ago. It ranks 133 of 158 by distance among the Van den Bergh nebulae. Distance source: Gaia DR3 parallax of the illuminating star via AT-HYG v3.2 (1142 pc).
