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Gomeisa — Star in Canis Minor

HIP 36188; Beta Canis Minoris; 3 Canis Minoris

Magnitude 2.9m Star Canis Minor (CMi) Visible
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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

Magnitude 2.90
Range 2.89 - 2.9
Period 7.4 hours
Variable Type Slowly Pulsating Be Star
Spectral Type B8Ve
Star Color Blue-white (B-V -0.09)
Distance 162 ly

2Position & Identifiers

RA 07h 27m 09.0s
Dec +08° 17' 22.0"
Constellation Canis Minor (CMi)
HR 2845
HIP 36188
HD 58715
SAO 115456
Bayer Beta
Flamsteed 3 CMi
Variable ID Bet CMi

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Easy Easy
50mm finder Easy Easy Easy
150mm scope Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

4Visibility

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Best season Dec – Feb (peak: Jan)

5Survey Image

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Explore

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Size Comparison

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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.

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Stellar Fusion

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15Stellar Notes

Gamma Cas 2.84 - 2.92V.
Rotationally unstable Be shell star.
Gomeisa; Algomeyla; Gomelza.
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Light Travel Time Machine

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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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