Menu

Spica

HIP 65474; Alpha Virginis; 67 Virginis

HIP 65474; Alpha Vir; 67 Vir DoubleStar Virgo (Vir) Visible
Star Map
+ List + Plan Back

About Spica

Description

Spica is a blue giant of spectral type B1III-IV at magnitude 0.98, the brightest star in Virgo and the 16th brightest in the sky. Located about 250 light-years from Earth, it is actually a close binary system — two hot stars orbiting every 4 days, so close they are distorted into egg shapes by tidal forces. The combined luminosity is about 12,100 times solar.

Observing Tips

Follow the arc of the Big Dipper's handle past Arcturus to 'speed on to Spica' — extending the arc about the same distance. Spica is a brilliant blue-white star low in the spring sky, marking the sheaf of wheat held by the Virgin. It is a useful guide to the Virgo Cluster of galaxies, which lies about 10° to the northwest. Best observed April through July.

History

The name Spica means 'ear of grain' in Latin, referring to the sheaf of wheat in the constellation figure. Hipparchus used observations of Spica around 130 BC to discover the precession of the equinoxes — one of the most important discoveries in ancient astronomy. Copernicus also used Spica to calibrate his observations.

Fun Facts

Spica is a rotating ellipsoidal variable — the two tidally distorted stars present different cross-sections as they orbit, causing tiny brightness changes. Both stars are so hot and massive that they will end their lives as supernovae, possibly leaving behind a double neutron star or even a black hole binary.

Observe

1Physical Properties

Magnitude 0.98
Range 0.96 - 1.00
Period 4.0 days
Variable Type Ellipsoidal Variable
Spectral Type B1IV
Star Color Blue (B-V -0.23)
Temperature 25412 K
Radius 7.4 R☉
Distance 250 ly

Position & Identifiers

RA 13h 25m 11.6s
Dec -11° 09' 41.0"
Constellation Virgo (Vir)
HR 5056
HIP 65474
HD 116658
Bayer Alpha
Flamsteed 67 Vir
Variable ID Alp Vir

2How easy to split?

Primary 1.0 mag Companion 12.0 mag Separation 151.9″
Sign in and configure your equipment and default location to see a personalized row.
Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. V. hard+ V. hard+ V. hard
150mm Newt. Medium Hard+ Hard
C8 203mm Medium+ Medium Hard+
Easy Medium Hard Very hard Impossible

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

3Visibility

Set a location in User Settings to see visibility data.

Best season Mar – May (peak: Apr)

4Light Curve

5Multiple 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

Log in to set your own equipment
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: 2.3″

Explore

7

Size Comparison

8

Compare Stars

9

Stellar Lifecycle

10

Spectral Classification

11

Hertzsprung-Russell Diagram

Loading HR diagram…
12

Blackbody Spectrum

13

Stellar Absorption Spectrum

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

14

Stellar Fusion

Discover

15Stellar 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".
16

Light Travel Time Machine

17

Relativistic Travel

Survey Image

Loading survey image…

Nearby in the Sky

Other targets within a few degrees — pan your scope a little and keep exploring.

}