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Pi Orionis — Star in Orion

HIP 22549; Pi Orionis; 3 Orionis

Magnitude 3.7m Star Orion (Ori) Visible
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About Pi Ori

Description

Pi3 and Pi4 Orionis are two separate hot B-type stars in Orion's shield region — Pi2 retains its Bayer designation at magnitude 3.69. The star cataloged as BS1552 is Pi-2 Orionis, a B2 III giant about 1,050 light-years away. It shines at magnitude 3.69 and is a member of the Orion OB1 stellar association. The star has estimated mass of 10 solar masses and is a source of X-rays from its fast stellar wind.

Observing Tips

Pi-2 Ori is one of the shield stars of Orion. Use binoculars to trace the whole arc of shield stars; Pi-2 appears crisp and blue-white. Best observed November through March.

History

Pi-2 Orionis has no widely-used traditional name in current IAU catalogs.

Fun Facts

Pi-2 Ori is a member of the vast Orion OB1 association — the closest young massive-star association to the Sun, extending across most of the constellation. Its stellar wind contributes to heating and ionizing the surrounding interstellar gas.

Observe

1Physical Properties

Magnitude 3.69
Spectral Type B2III giant
Star Color Blue (B-V -0.17)
Distance 1,048 ly

2Position & Identifiers

RA 04h 51m 12.4s
Dec +05° 36' 18.0"
Constellation Orion (Ori)
HR 1552
HIP 22549
HD 30836
SAO 112142
Bayer Pi
Flamsteed 3 Ori

3How easy to spot?

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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Easy Medium+ Medium+
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 Oct – Dec (peak: Nov)

5Survey Image

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Explore

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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.

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Stellar Fusion

Discover

15Stellar Notes

9.5191d, K 25.8k/s, V0 +23.3k/s, asini 3.38.
Ori OB1.
See HR 1543.
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Light Travel Time Machine

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Relativistic Travel

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