Star profile

11 Canis Minoris

3D likeness based on its real data · class A · ~8,500 K

What is 11 Canis Minoris

11 Canis Minoris peers out from the smaller of Orion's two dogs, a constellation dominated by the nearby brilliance of Procyon. It is a white A-type star with a surface markedly hotter than the Sun's, and its light takes a little over three hundred and one years to cross the void to us. Barely visible to the unaided eye, it demands a dark sky and patience to be picked out.

Where it is and when to see it

11 Canis Minoris lies in the northern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is January, when it culminates around midnight.

From London it culminates about 49° above the horizon.
From New York it culminates about 60° above the horizon.
From Sydney it culminates about 45° above the horizon.

It can be seen from anywhere north of 79° S.

It ranks no. 10 in brightness among the 25 stars of Canis Minor in our catalogue. To find it, start from Procyon, the brightest: it lies about 6° away (a fist at arm's length covers about 10°).

The light you see today left it about 300 years ago.

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Astronomical data for 11 Canis Minoris

Constellation: Canis Minor
Apparent magnitude: 5.25
Distance: 301.5 light years
Coordinates (J2000): RA 116.568° · Dec 10.768°
Catalogue: HIP 37921 · HD 62832

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Other stars in Canis Minor

Canis Minor has 25 stars in Stelvia's catalogue. Here are a few of them.

See all 25 stars in Canis Minor