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Tania Australis — Variable Star in Ursa Major

HIP 50801; Mu Ursae Majoris; 34 Ursae Majoris

Observable Variable Star Excellent (60/100)

Range: 3.03 - 3.10, Period: 230.1d, Type: EB:+LB

Magnitude 3.0–3.3m VariableStar Ursa Major (UMa) Visible
Star Map
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About Tania Australis

Description

Tania Australis (Mu Ursae Majoris) is a red giant of spectral type M0III at magnitude 3.05 in Ursa Major. Located about 230 light-years from Earth, it has a cool surface temperature of roughly 3,900 K and a distinctly orange-red color. It forms the southern member of the 'Tania' pair with Lambda UMa (Tania Borealis), representing one of the Bear's hind paws.

Observing Tips

Mu UMa lies below the Big Dipper's bowl, forming a close pair with Lambda UMa (Tania Borealis) about 2 degrees to its north. The two Tania stars make an attractive binocular pair with contrasting colors — Mu is orange-red while Lambda is white. They represent the Bear's southern hind foot. Best observed from February through July when Ursa Major is high overhead.

History

The name Tania Australis means 'the southern Tania' in Latin/Arabic hybrid form. 'Tania' derives from the Arabic 'al-thaniya,' meaning 'the second' (leap of the gazelle). The three pairs of stars in the Bear's feet (Talitha, Tania, and Alula) were seen in Arab astronomy as three successive leaps of a gazelle.

Fun Facts

The three pairs of stars forming the Great Bear's hind legs — Talitha (Iota/Kappa UMa), Tania (Lambda/Mu UMa), and Alula (Nu/Xi UMa) — were imagined in Arabic astronomy as the tracks of a bounding gazelle. Each pair represents one leap, creating a charming alternative interpretation of these stars.

Observe

1Physical Properties

Magnitude 3.05
Range 3.03 - 3.10
Period 230 days
Variable Type EB:+LB
Spectral Type M0III giant
Star Color Red (B-V 1.59)
Distance 230 ly

2Position & Identifiers

RA 10h 22m 19.7s
Dec +41° 29' 58.0"
Constellation Ursa Major (UMa)
HR 4069
HIP 50801
HD 89758
SAO 43310
Bayer Mu
Flamsteed 34 UMa

3How easy to follow?

Magnitude 3.0 – 3.3 mag Amplitude 0.3 mag Period 230.1 d Type EB:+LB
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Equipment Bortle 3 Bortle 4 Bortle 5
Naked eye Hard+ Hard+ Hard
50mm finder Hard+ Hard+ Hard+
150mm scope Hard+ Hard+ Hard+
Easy Medium Hard Very hard Impossible

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

Out of reach for typical amateur telescopes, even at Bortle 3.

4Visibility

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Best season Jan – Mar (peak: Feb)

5Survey Image

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6Light Curve

7Comparison Stars

Nearby stable stars for estimating brightness (AAVSO)

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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

17Stellar Notes

E?, 2.99 - 3.33V.
230.089d, K 7.4k/s, V0 -20.4k/s, asini 23.4.
Ultraviolet FeII emission. H and K emission.
Tania Australis.
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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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