Astrophysics (index)

Color Index

(a number that characterizes the color of an object)

An object's Color Index is its difference in Magnitude as seen through two different filters, such as B versus V, or U versus B, typically with the Passbands standardized by the UBV Photometric System. The most commonly-cited color index, B-V, is a star's magnitude as observed through the B filter minus its magnitude through the V filter. A star's Effective Temperature (Teff) can be estimated from B-V. The color index U-B is also commonly noted.

A color index is analogous to a human's perception of color in the following manner: the Wavelengths perceived as "blue" are also present when the colors "white" or "gray" are perceived. We perceive the color blue when the ratio of the Intensity in the blue wavelengths to the others (red, green, etc.) is high. Like this, color indexes, being differences in magnitude, express ratios of the intensity of different wavelength-ranges.

The color index reflects properties of the observed star, being generally unchanged by distance, making it a primary basis for analysis for stars too far for Spectroscopy. However, the Observed Color Index can be affected by properties of intervening matter. This effect is quantified by the Color Excess (EB-V), which is a star's actual (Intrinsic or Normal) color index minus its observed color index.

EB-V = (B-V)Observed - (B-V)Intrinsic

A good estimate of the color excess increases the accuracy and value of a star's color index.


Referenced by:
AD Leonis (AD Leo)
Algol (Beta Per)
Alpha Centauri
Aperture Photometry
Barnard's Star
Balmer-Break Galaxy (BBG)
Beta Centauri
Color-Color Diagram
Color-Period Diagram
Epsilon Eridani
Epsilon Indi (ε Indi)
HR 8799
Lacaille 9352
Lalande 21185
Luyten 726-8
Main Sequence Fitting
Mass-Radius Relation
Photometric System
Ross 154
Ross 248
Stellar Radius Determination
T Tauri
UBV Photometric System
Wolf 359