About Bharani
Description
Bharani, 41 Arietis, is a B-type main-sequence star of spectral class B7 V about 166 light-years away. It shines at magnitude 3.63 and is one of the brighter stars in Aries. Bharani is part of the Pleiades Moving Group — a loose stellar stream sharing common motion with the Pleiades cluster — and is about 50 million years old.
Observing Tips
Bharani sits east of Hamal (Alpha Ari) in the eastern part of Aries. In binoculars its blue-white color stands out clearly. Best observed October through February.
History
The name Bharani comes from Sanskrit, referring to the second of the 27 nakshatras (lunar mansions) of Indian astronomy. The Bharani nakshatra corresponds to this region of Aries. The IAU adopted the name in 2017.
Fun Facts
Bharani is one of several IAU-adopted star names drawn from the Sanskrit nakshatra tradition. The 27 nakshatras form a parallel Indian zodiac system, dividing the ecliptic into equal lunar-month-based segments rather than the 12 solar-month-based signs of the Western zodiac.
Observe
1Physical Properties
2Position & Identifiers
3How easy to spot?
| Equipment | Bortle 3 | Bortle 4 | Bortle 5 |
|---|---|---|---|
| Naked eye Naked eye | Easy | Medium+ | Medium+ |
| 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
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5Survey Image
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Explore
7
Size Comparison
8
Compare Stars
9
Spectral Classification
10
Hertzsprung-Russell Diagram
11
Stellar Lifecycle
12
Blackbody Spectrum
13
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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