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Spica

HIP 65474; Alpha Vir; 67 Vir

HIP 65474; Alpha Vir; 67 Vir DoubleStar Vir Visible Level 3 Medium telescope (6-8") - Requires steady seeing
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Physical Properties

Magnitude 0.98
Variable Type Beta Cephei (Pulsating)
Spectral Type B1IV
Star Color Blue (B-V -0.23)
Temperature 25412 K
Radius 7.4 R☉
Distance 249.9 ly

Position & Identifiers

RA 13h 25m 11.6s
Dec -11° 09' 41.0"
Constellation Vir
HR 5056
HIP 65474
Bayer Alpha
Flamsteed 67 Vir
Variable ID Alp Vir

Visibility

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Multiple Star System

Components 5
Component IDs O
Separation 151.9″
Companion Mag 12.0
Companion Sp B2
Position Angle 33°
Star Colors A: Blue B: Blue
Discoverer BUP 150

Eyepiece View

80x Dawes: 1.9″ TFOV: 0.6°
Realistic = true angular size
N E 33° A (1.0) B (12.0)

Sep: 151.9″ · PA: 33° · N up, E left

Resolved · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″

Size Comparison

Stellar Lifecycle

Spectral Classification

Hertzsprung-Russell Diagram

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Blackbody Spectrum

Stellar Absorption Spectrum

Simulated absorption spectrum based on spectral type. Hover over lines to identify elements.

Stellar Notes

Ell (Beta C) 0.97 - 1.04V, 4.01454d, and Beta C, 0.1737853d. Period changes.
Interferometer indicates visual component A is multiple system. Occultations yield three companions: 3.1v at 0.0025", | 4.5 at 0.05" and 7.5 at 0.5". Combined mag. and colors. Visual component B, 12.0v at 148".
4.0145d, K 120k/s, V0 0k/s, msin3i 7.16, asini 6.52. Rotation apsides 130 yrs. Rotational velocity 190k/s. | vsini secondary 102k/s.
Color excess E(B-V) = +0.03.
Also variously classified B2V+B2V, B1.5IV-V+B3V, B1V+B3V. Rocket observations show hydrogen lines Lyman alpha | through Zeta.
SPICA; Azimech; Spica Virginis; Alaraph, a name also given HR 4540, 4932.
Diam. = 0.00085 - 0.00087".

Survey Image

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About Spica

Description

Spica is the brightest star in Virgo and the 15th brightest in the night sky at magnitude 0.98. It is a blue giant of spectral type B1III-IV, located about 250 light-years from Earth. Spica is actually a close spectroscopic binary: two hot stars orbiting each other every 4.01 days at a separation of only about 0.12 AU. The primary is about 10 times the mass of the Sun and 12,000 times more luminous. The two stars are so close that they are tidally distorted into egg shapes.

Observing Tips

Spica is easy to find using the arc-to-Arcturus, spike-to-Spica mnemonic — follow the arc of the Big Dipper's handle through Arcturus and continue the curve to reach Spica. Its blue-white color contrasts sharply with the orange of nearby Arcturus. Spica is a useful reference star for the zodiac, as planets and the Moon frequently pass near it along the ecliptic. Best observed from March through July.

History

The name Spica comes from the Latin 'Spica Virginis' meaning 'ear of grain,' as it represents the sheaf of wheat held by the constellation Virgo. Hipparchus used observations of Spica around 130 BC to discover the precession of the equinoxes — one of the most important discoveries in ancient astronomy. Nicolaus Copernicus also observed Spica to refine his understanding of precession.

Fun Facts

The two stars of Spica are so close together that they are tidally distorted into ellipsoidal shapes, causing the system's brightness to vary by about 0.03 magnitudes as the elongated stars present different cross-sections to our line of sight. Spica is one of the 'pointer stars' for navigators and was critical to the discovery of precession over 2,000 years ago.