Glossary

Astronomy glossary

514 definitions · page 4 of 9.

focal ratio (f ratio)
the ratio of the focal length of a lens or mirror to its diameter
focal ratio (f ratio):
the ratio of the focal length of a lens or mirror to its diameter
focus
the point at which rays of light passing through a lens (or reflecting off a mirror) converge
focuser
the device on a telescope that holds an eyepiece and moves to allow an observer to bring light to a sharp focus
fork mount
an equatorial mount in which the telescope swings in declination between the two prongs of a fork
frequency
the number of wave crests or troughs that pass a particular point in a given interval of time (usually one second); usually expressed in hertz (cycles per second)
full moon
the phase of the moon when it is halfway around its orbit from new moon and opposite the sun in the sky; the full disk is illuminated
galactic disk
the disk of a spiral galaxy
galactic nucleus
the central region of a galaxy; often contains a high density of stars and gas, and a supermassive black hole
galactic plane
the projection of the Milky Way’s disk on the sky.
galaxy
an enormous gravitationally bound assemblage of millions or billions of stars
galaxy cluster
a gravitationally bound assemblage of dozens to thousands of galaxies
Galilean moons
Jupiter's four largest moons: Io, Europa, Ganymede, and Callisto; discovered by Galileo Galilei in 1610
Galilean satellites
Jupiter's four largest moons: Io, Europa, Ganymede, and Callisto; discovered by Galileo Galilei in 1610
gamma rays
the form of light (electromagnetic radiation) with the shortest wavelength and the most energy
gamma-ray burst
a short, intense burst of high-energy radiation emanating from the distant universe
gas giant
a large planet made primarily of gas, such as Jupiter, Saturn, Uranus, and Neptune
general relativity
the theory of relativity governing accelerated motion that describes gravity as a curvature of space-time
german equatorial mount
a mount in which the declination axis sits on top of the polar axis, with the telescope on one end of the declination axis and a counterweight on the other
giant molecular cloud
interstellar clouds of cold gas and dust that contain tens or hundreds of thousands of solar masses
gibbous
the phase of the moon between first quarter and last quarter, when the moon appears more than half illuminated
globular cluster
a roughly spherical congregation of hundreds of thousands of stars; most globular clusters consist of old stars and exist in a galaxy’s halo
gravitational lens
a massive object which magnifies or distorts the light from a more distant object along the same line of sight
gravitational lensing
the distortion or amplification of an object’s light due to the presence of a massive object in the light path
gravitational waves
weak, wavelike disturbances which represent the radiation related to the gravitational force; produced when massive bodies are accelerated or otherwise disturbed
gravity
the attractive force that all objects exert on one another; the greater an object’s mass, the stronger its gravitational pull
gravity waves
weak, wavelike disturbances which represent the radiation related to the gravitational force; produced when massive bodies are accelerated or otherwise disturbed
habitable zone (or ecosphere)
the zone around a star in which a planet can maintain liquid water on its surface
halo
the outer region of a galaxy; contains globular clusters, a few stray stars, and dark matter
heliacal rising
the period of time when an object, such as a star, is briefly seen in the eastern sky before dawn and is no longer hidden from the glare of the sun
heliosphere
a vast region around the sun dominated by the solar wind
helium
the second lightest element; consists of two protons, and usually two neutrons and two electrons; about 8 percent of the atoms in the universe are helium
Hertz
a unit of frequency equal to one cycle per second
HII region
an area filled with clouds of ionized hydrogen; the ionization is usually caused by radiation from newborn stars
HST
The Hubble Space Telescope makes its observations from above Earth's atmosphere. The telescope orbits 600 kilometers (375 miles) above Earth, working around the clock. It was originally designed in the 1970s and launched in 1990. The telescope is named for…
Hubble law
the principle that a distant galaxy’s recessional velocity is proportional to its distance from Earth
Hubble Space Telescope
The Hubble Space Telescope makes its observations from above Earth's atmosphere. The telescope orbits 600 kilometers (375 miles) above Earth, working around the clock. It was originally designed in the 1970s and launched in 1990. The telescope is named for…
hydrazine
a colorless liquid which burns rapidly and is used as a common rocket and missile fuel
hydrogen
the simplest and lightest element; usually consists of just a single proton and electron; about 90 percent of the atoms in the universe are hydrogen
hypered film
ilm that has been treated, usually with gas, to enhance its response to low light levels
igneous rock
rock formed by the solidification of magma
inclination
the angle between a planet’s orbit and the ecliptic plane; or the angle between a satellite’s orbit and its host planet’s rotational plane
inferior conjunction
the configuration of an inferior planet when it lies between the sun and Earth
inferior planet
a planet that orbits the sun inside of Earth’s orbit; includes Mercury and Venus
inflation
a brief and extraordinarily rapid period of expansion a fraction of a second after the Big Bang
infrared
a form of light with slightly lower energy than visible light but with greater energy than radio waves
interacting galaxies
galaxies caught in each other’s gravitational embrace, often results in galactic mergers or extreme star formation
interference fringes
a wave-like pattern resulting from the successful combination of two beams of light which amplifies the light
interferometer
a system of two or more widely separated telescopes that achieves the resolving power of a much larger telescope
interferometric fringes
a wave-like pattern resulting from the successful combination of two beams of light which amplifies the light
interferometry
the technique of using two or more widely separated telescopes to achieve the resolving power of a much larger telescope
intergalactic
the space between the galaxies
International Space Station
a global cooperative program between the United States, Russia, Canada, Japan, and Europe, for the joint development, operation, and utilization of a permanently habitated space station in low-Earth orbit
interplanetary
the space between the planets
interstellar
the space between the stars of a galaxy
interstellar medium
the gas and dust located between the stars
ion
an atom that is electrically charged due to the loss or gain of one or more electrons
ionization
the process by which an atom gains or loses electrons
ionized gas
a gas that has been heated to a state where it contains ions and free-floating electrons; also known as a plasma
ionosphere
an atmospheric layer with a high concentration of ions and free electrons