Gomeisa — Star in Canis Minor
HIP 36188; Beta Canis Minoris; 3 Canis Minoris
About Gomeisa
Description
Gomeisa is a blue-white main-sequence star of spectral type B8Ve at magnitude 2.90, the second brightest star in Canis Minor. Located about 162 light-years from Earth, it has a luminosity of roughly 250 times solar. It is a Be star, rapidly rotating and occasionally ejecting gas into a circumstellar disk.
Observing Tips
Gomeisa lies about 4 degrees northwest of brilliant Procyon in the small constellation Canis Minor. It is a blue-white star providing a color contrast with the yellow-white Procyon. Canis Minor contains only these two bright stars. Best observed January through April.
History
The name Gomeisa comes from the Arabic 'al-ghumaisa,' meaning 'the bleary-eyed one.' In Arabic tradition, Gomeisa and Procyon were 'the two sisters' who wept for their brother (Sirius) who had crossed the Milky Way.
Fun Facts
Canis Minor is one of the smallest constellations, and essentially consists of just Procyon and Gomeisa — a contrast between a nearby yellow-white star and a distant hot blue star that happen to lie in almost the same direction from Earth.
Observe
1Physical Properties
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Easy | Easy |
| 50 mm finder 50mm finder | Easy | Easy | Easy |
| 150 mm telescope 150mm scope | Easy | Easy | Easy |
Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs
4Visibility
Set a location in User Settings to see visibility data.
5Survey Image
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Explore
7
Size Comparison
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Compare Stars
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Spectral Classification
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Hertzsprung-Russell Diagram
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Stellar Lifecycle
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Blackbody Spectrum
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Stellar Absorption Spectrum
Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.
14
Stellar Fusion
Discover
15Stellar Notes
16
Light Travel Time Machine
17
Relativistic Travel
Nearby in the Sky
Other targets within a few degrees — pan your scope a little and keep exploring.
Visibility scores assume a 150 mm Newton at Bortle 4.
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