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Tianguan — Star in Taurus

HIP 26451; Zeta Tauri; 123 Tauri

Magnitude 2.9–3.0m Star Taurus (Tau) Visible
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About Tianguan

Description

Zeta Tauri is a blue star of spectral type B4IIIpe at magnitude 3.0 in Taurus. Located roughly 440 light-years from Earth, it marks the tip of the Bull's southern horn. The 'pe' in its spectral classification indicates it is a shell star — a rapidly rotating star surrounded by a disk of expelled gas. It is also a spectroscopic binary.

Observing Tips

Zeta Tau marks the southern horn tip of Taurus, forming a pair with Beta Tau (Elnath) at the northern horn tip. It is easy to find by following the line of Orion's Belt to the upper left (northwest). The Crab Nebula (M1) lies about 1 degree to the northwest of Zeta Tau, making this star the primary guide for finding one of the most famous deep-sky objects. Best observed from November through March.

History

Zeta Tauri has no widely used traditional proper name, though it has occasionally been called Tianguan in Chinese astronomy, meaning 'celestial gate.' Its proximity to the Crab Nebula (M1) is historically significant — the 1054 supernova that created the Crab Nebula was recorded very close to this star's position.

Fun Facts

Zeta Tau is the most important guide star for finding the Crab Nebula (M1). When Chinese astronomers recorded the 'guest star' of 1054, they described its position relative to Zeta Tau. As a shell star, Zeta Tau's equatorial disk causes its spectrum to show emission lines that vary over time as the disk changes.

Observe

1Physical Properties

Magnitude 3.00
Range 2.8 - 3.17
Period 133 days
Variable Type E/GS+GCAS
Spectral Type B1IVe shell supergiant
Star Color Blue (B-V -0.19)
Distance 438 ly

2Position & Identifiers

RA 05h 37m 38.7s
Dec +21° 08' 33.0"
Constellation Taurus (Tau)
HR 1910
HIP 26451
HD 37202
SAO 77336
Bayer Zeta
Flamsteed 123 Tau
Variable ID Zet Tau

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 Nov – Jan (peak: Dec)

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

Discover

15Stellar Notes

Gamma Cas 2.90 - 3.03V. Var. shell Sp. Widths H-lines vary in about 10 min. Polarization at H beta changes in tens | of minutes, probably due to circumstellar matter.
132.91d, K 8.9k/s, V0 +21.8k/s, asini = 16.1. 3.2, 5.2v, sep. 0.007". Common circumstellar envelope. The 132.9d | period is superimposed on a 7y pseudo-period related to oscillation of envelope.
Color excess E(B-V) = +0.09.
Cas-Tau OB1.
Lyman beta observed from COPERNICUS. Spectra obtained from AEROBEE rocket show absorption features at 1920 (FeIII) | and 1720A (AlII) associated with extended atmosphere or circumstellar shell. Also classified B2IVp.
Rapidly rotating star. Rotational velocity varies with wavelength: vsini about 300k/s in visual, 150 or less in UV. | Expanding circumstellar shell. Shell-line velocities do not correspond to orbital elements; possibly gaseous ring. | Unstable shell star with pseudo-periodic phenomena.
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Light Travel Time Machine

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Relativistic Travel

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