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Maia — Star in Taurus

20 Tau

Magnitude 3.9m Star Taurus (Tau) Visible
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About Maia

Description

Maia, 20 Tauri, is a B6.5 III giant about 399 light-years away and one of the brightest stars of the Pleiades open cluster (M45). At magnitude 3.87 it is the fourth-brightest Pleiad. Maia has a mass of about 5 solar masses and rotates slowly for a B-type star. Like several of its cluster siblings, Maia is embedded in a reflection nebula — a dusty remnant lit up by the star's blue light, cataloged as NGC 1432 and also known as the Maia Nebula.

Observing Tips

Maia is one of the "Seven Sisters" — readily visible to the naked eye as one of the defining points of the Pleiades asterism. In a 4-inch or larger telescope under dark skies, the nebulosity surrounding Maia becomes visible as a soft blue glow enveloping the star. Best observed October through March.

History

Maia is named for one of the Pleiades of Greek mythology — the eldest of the Seven Sisters, daughters of Atlas and Pleione. The name is one of the oldest continuously used star-names in Western astronomy, traceable to Homer and Hesiod. The reflection-nebula association was first photographed at Paris Observatory in 1885.

Fun Facts

The Maia Nebula (NGC 1432) is part of the larger interstellar dust cloud that the Pleiades is currently passing through — the nebulosity is not cluster-native but a chance encounter. The star also gives its name to the "Maia variables," a now-defunct variable-star class originally proposed in the 1950s but later shown not to be a distinct population.

Observe

1Physical Properties

Magnitude 3.87
Spectral Type B6.5III giant
Star Color Blue-white (B-V -0.07)
Distance 399 ly

2Position & Identifiers

RA 03h 45m 49.6s
Dec +24° 22' 04.0"
Constellation Taurus (Tau)
HR 1149
HIP 17573
HD 23408
SAO 76155
Flamsteed 20 Tau

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

Probably cst. Var. helium lines.
Sep. 0.003". Unresolved by speckle interferometry 1981.69. Duplicity questioned.
Color excess E(B-V) = +0.02.
Pleiades cluster; Mel 22 #785; in reflection nebula. Pleiades nebula. Member assoc. Tau R1 at 110 pc.
C1 neutral carbon continuum shows discontinuities in UV.
Maia.
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Light Travel Time Machine

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Relativistic Travel

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