Long wave UV - Ultraviolet light with wavelengths (about 10 -7 meters) just shorter than the optical range of the electromagnetic spectrum.

Microwaves - Electromagnetic radiation with wavelengths ranging around 10 -3 meters.

Nanometer - One billionth of a meter (10 -9 m).

Neutron stars - A star about 10 kilometers in diameter composed entirely of densely-packed neutrons.

Objective lens or mirror - The large lens or mirror of a telescope. Sometimes referred to as the primary lens or mirror.

Ozone layer - A region in Earth's upper atmosphere (between 15 and 30 kilometers) where small concentrations of ozone absorb ultraviolet radiation from the Sun and other celestial bodies.

Persistence of vision - Momentary visual retention of light.

Photometry - Measurement of the intensity of light.

Photons - A quantum or individual packet of electromagnetic energy.

Photosphere - The visible surface of the Sun.

Pixels - The smallest element of a picture.

Pulsars - A stellar radio source that emits radio waves in a pulsating rhythm.

Radio waves - Electromagnetic radiation with wavelengths ranging from approxi-mately 10 4 to 10 -2 meters.

Refraction - Bending of light rays as they

pass through the interface between two transparent media.

Resolution - The degree to which fine details in an image can be seen as separated or resolved.

Resonance - Sympathetic vibration of one body when exposed to vibrations or electromagnetic radiation emanating from another.

Scientific Notation - Scientific notation, or powers of 10, which can simplify writing large numbers. Numbers with positive powers mean the decimal point moves to the right (e.g., 3 x 106 = 3,000,000). A number with a negative power means that the decimal moves to the left (e.g., 3 x 10 -6 = 0.000,006).

Short wave UV - Ultraviolet light with wavelengths nearest the x-ray range (around 10 -8 meters) of the electromagnetic spectrum.

Space-based astronomy - Astronomical investigations conducted from above Earth's atmosphere.

Spectrograph - An instrument used for dispersing and recording specific wavelengths of the electromagnetic spectrum.

Spectroscopy - The study of spectra.

Speed of light - The speed at which light travelsQ300,000,000 meters per second.

Supernova - A stellar explosion which increases the brightness of a star by a factor of several million times in a matter of days.

Ultraviolet (UV) - Electromagnetic radiation with wavelengths ranging from

Next page Teacher Resources


Last modified prior to September, 2000 by the Windows Team

The source of this material is Windows to the Universe, at http://windows2universe.org/ from the National Earth Science Teachers Association (NESTA). The Website was developed in part with the support of UCAR and NCAR, where it resided from 2000 - 2010. © 2010 National Earth Science Teachers Association. Windows to the Universe® is a registered trademark of NESTA. All Rights Reserved. Site policies and disclaimer.