An Etymological Dictionary of Astronomy and Astrophysics

The inner part of the → solar corona which extends to about two solar radii. It is due to the → Thomson scattering of light from the → photosphere by the free electrons in the corona. The K corona exhibits a → linearly polarized continuous spectrum. The high speeds of the scattering electrons (on the average 10,000 km s^-1 for a temperature of 2 million K) smear out the → Fraunhofer lines except the → H and K lines.

See also: K from Ger. Kontinuum, → continuum; → corona.

The inner part of the → solar corona which extends to about two solar radii. It is due to the → Thomson scattering of light from the → photosphere by the free electrons in the corona. The K corona exhibits a → linearly polarized continuous spectrum. The high speeds of the scattering electrons (on the average 10,000 km s^-1 for a temperature of 2 million K) smear out the → Fraunhofer lines except the → H and K lines.

See also: K from Ger. Kontinuum, → continuum; → corona.

A → color index correction applied to the photometric magnitudes and colors of a distant galaxy to compensate for the “reddening” of the galaxy due to → cosmological redshift. K correction is intended to derive the magnitudes in the → rest frame of the galaxy. Typically it is given as K(z) = az + bz², where a and b depend on galaxy types. Conversely, one may deduce the redshift of a galaxy by its colors and a K-correction model.

See also: The term K correction, probably stems from the K-term used by C. W. Wirtz (1918, Astron. Nachr. 206, 109), where K stands for Konstante,
the German word for constant. The K-term was a constant offset in the redshift applied to diffuse nebulae in that epoch (source: A. L. Kinney, 1996, ApJ 467, 38);
→ correction.

A → color index correction applied to the photometric magnitudes and colors of a distant galaxy to compensate for the “reddening” of the galaxy due to → cosmological redshift. K correction is intended to derive the magnitudes in the → rest frame of the galaxy. Typically it is given as K(z) = az + bz², where a and b depend on galaxy types. Conversely, one may deduce the redshift of a galaxy by its colors and a K-correction model.

See also: The term K correction, probably stems from the K-term used by C. W. Wirtz (1918, Astron. Nachr. 206, 109), where K stands for Konstante,
the German word for constant. The K-term was a constant offset in the redshift applied to diffuse nebulae in that epoch (source: A. L. Kinney, 1996, ApJ 467, 38);
→ correction.

An orange-red star of → spectral type K with a surface temperature of about 3600-5000 K. The spectra of K stars are dominated by the H and K lines of calcium and lines of neutral iron and titanium, with molecular bands due to cyanogen (CN) and titanium dioxide (TiO). Examples are → Arcturus and → Aldebaran.

See also: K the letter of alphabet; → star.

An orange-red star of → spectral type K with a surface temperature of about 3600-5000 K. The spectra of K stars are dominated by the H and K lines of calcium and lines of neutral iron and titanium, with molecular bands due to cyanogen (CN) and titanium dioxide (TiO). Examples are → Arcturus and → Aldebaran.

See also: K the letter of alphabet; → star.

Same as the → Cretaceous-Tertiary event.

See also: K, representing the “→ Cretaceous period,” and T the “→ Tertiary;” → event.

Same as the → Cretaceous-Tertiary event.

See also: K, representing the “→ Cretaceous period,” and T the “→ Tertiary;” → event.

A follow-up mission of the → Kepler satellite funded by → NASA. K2 provides an opportunity to continue Kepler’s observations in the field of → exoplanets and expand its role into new astrophysical observations by assigning to Kepler new mission.

See also: K, short for → Kepler spacecraft; 2, for second → mission.

A follow-up mission of the → Kepler satellite funded by → NASA. K2 provides an opportunity to continue Kepler’s observations in the field of → exoplanets and expand its role into new astrophysical observations by assigning to Kepler new mission.

See also: K, short for → Kepler spacecraft; 2, for second → mission.