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TERMINOLOGY / GLOSSARY |
Term Description:
| Altitude | Angular distance, usually measured in degrees, above the horizon |
| Aphelion | The point farthest from the sun in an object's orbit |
| Apogee | The point in a satellites orbit when it is farthest from the Earth |
| Apparent Magnitude | A measure of the brightness of a celestial object as seen by an observer; brighter objects have smaller numerical magnitudes. |
| Asterism | A notable pattern of stars, such as the Big Dipper, forming part of a constellation; not a constellation itself. |
| Asteroids | Small, rocky objects that orbit the Sun; mainly between Mars and Jupiter |
| Astronomical Unit | Unit of measurement, abbreviated AU, that is the distance between the Earth and the Sun; 93 million miles |
| Averted Vision | An observing trick of looking at an object in the eyepiece is to look a little to one side of the target. This "averted vision" places the target on a more light-sensitive area of the eye's retina where it will pop into view. |
| Azimuth | A celestial object's distance from true north measured eastward in degrees along the horizon |
| Binary Stars | A double star system; two (or more) stars revolving about a common center of gravity |
| Black Hole | A collapsed massive star; so dense that not even light can escape the pull of its gravity |
| Brown Dwarf | A star with insufficient mass to initiate a fusion reaction |
| Cassegrain Telescope | A reflecting telescope in which a secondary mirror reflects light back through a hole in the center of the primary mirror. |
| Catalogues | Lists of stars and deep sky objects, i.e., M11 (Messier Object No. 11); NGC (New General Catalog); IC (Index Catalog); SAO (Smithsonian Astrophysical Observatory); GCVS (General Catalog of Variable Stars) |
| Celestial Equator | The projection onto the sky of the Earth's equator. |
| Celestrial Pole | The projection of Earth's north and south pole axes onto the celestrial sphere. |
| Celestrial Sphere | An imaginary hollow sphere surrounding the Earth on which the stars appear to be fixed. |
| Circumpolar | The stars or constellations that are closer to the celestial pole than the horizon and therefore never set |
| Comets | A body, probably resembling a "dirty snowball" between 0.1 and 100 miles across that travels through the solar system in an elliptical orbit of random inclination. A comet grows a tail if it comes close enough to the sun. |
| Conjunction | The alignment or close alignment of two or more astronomical bodies. |
| Constellation | One of 88 recognized star figures into which the sky is divided; also refers to the historical, mythological or other figures that represented earlier divisions of the sky. |
| Coordinate System | The use of Right Ascension and Declination to locate an object in the sky. |
| Corona | The outermost layer of the sun and many other stars; a faint halo of extremely hot (million-degree) gas |
| Crater | The impression left in a surface of solid planets or moons by the impact of meteorite, asteroid or comet |
| Dark Skies | Prime sky conditions for viewing without light pollution from moon or man |
| Dark Matter | A form of matter that exerts gravitation force but does not emit any detectable light or radiation; dark matter comprises most of the mass of the universe but its exact nature remains unknown |
| Dark Nebula | A dust cloud blocking the light from behind. |
| Dec | Abbreviation of Declination, which along with Right Ascension determines a position on the sky. Declination is measured north (+) and south (-) from the celestial equator and specified in degrees and minutes. |
| Declination | The angular distance of a celestial object above or below the celestial equator; the celestial sphere equivalent of latitude |
| Diffuse Nebula | An Emission or Reflection nebula |
| Dust | Micron-size solid particles of somewhat uncertain composition, probably carbon, iron or silicates. |
| Dwarf Star | The remnant core of a sun-like star, which is extremely small, hot and dense |
| Ecliptic | The plane of Earth's orbit around the sun; all the planets except for Mercury and Pluto have orbits in nearly virtually the same plane |
| Elongation | Apparent angular distance of a member of the solar system from the sun as seen from the earth. |
| Emission Nebula | A gas cloud radiating by stimulated emission. |
| Galactic Cluster | A loose cluster of small number of stars; aka Open Cluster. |
| Galaxy | A large system of millions to hundreds of billions of stars; sometimes containing large amounts of dust and gas. Our Galaxy is called the Milky Way. |
| Globular Cluster | An ancient, spherical, densely populated cluster in orbit around the galaxies halo |
| Great Rift | From Cygnus to Aquilla, the Milky Way appears to be divided lengthwise by enormous dust clouds. |
| Great Red Spot | A high altitude storm cloud on Jupiter that was first observed in the 1600s |
| Greatest Elongation | When a planet attains its greatest apparent angular distance from the sun in the sky. |
| Inferior | Inferior conjunction is when an "inferior planet" (Mercury or Venus) passes between the earth and the sun. |
| Inferior Conjunction | The place in which a planet whose orbit is inside that of the Earth, passes between the Earth and the Sun |
| Light Pollution | Light, typically from artificial sources, that reaches the night sky, obscuring the view of faint astronomical object |
| Light Year | The distance light travels in a year - about 6 trillion miles. |
| Lunar Eclipse | The passage of the moon into the earth's shadow |
| LY | Abbreviation for Light-Year |
| Magnitude | Astronomical measurement of the brightness of an object; the lower the number, the bright the object |
| Main Sequence Star | A star in the prime of its life; where hydrogen inside is undergoing nuclear fusion |
| Meridian | A great circle on the celestial sphere passing through the north and south celestial poles and the zenith (overhead point) of a given place |
| Messier | Charles Messier was a French Comet Hunter. His catalog (first published in 1781) of nebulous objects was originally intended as a list of "junk" to avoid when searching for comets. |
| Meteor | A track of light in the sky resulting from the vaporization of solid matter entering the earth's atmosphere; commonly called "shooting stars" or "falling stars" |
| Meteor Shower | The appearance of many meteors during a short period of time; as when the earth passes through a comet's orbit |
| Meteorite | The part of a meteor that survives its passage through the earth's atmosphere |
| Milky Way | The name of our Galaxy in which our Solar System is located; the band of light that encircles the entire sky and stretches from horizon to horizon that results from the combined light of billions of stars in the Galaxy's disk |
| Moon | A smaller body orbiting a larger body; often refers to Earth's moon |
| Nebula | Any of various types of extended objects in the sky; see individual names. |
| Nebulae | Plural form of "nebula" |
| Neutron Star | A collapsed, extremely dense star (i.e., a billion tons per cubic centimeter) consisting almost entirely of neutrons; the final state of a star about twice as massive as the sun |
| NGC | New General Catalogue, compiled by JLE Dreyer in 1888; later amended by the two Index Catalogues (IC) |
| Northern Lights | The emission of light when charged particles from the solar wind, caused by magnetic storms on the sun, slam into and excite atoms and molecules in the Earth's upper atmosphere |
| Nova | A star that suddenly flares in brightness by a factor of hundreds of thousands |
| Occulation | The eclipse of one celestial object by another; as when the moon or a planet passes in front of a star. |
| Old | An old star is very old indeed, about 10- billion years or more. |
| Oort Cloud | A vast spherical halo of icy objects around the solar system; the repository of long period comets |
| Open Cluster | A irregular, loose cluster of stars of common origin; found in the spiral arms of the Galaxy |
| Opposition | The moment when a planet farther from the sun than the Earth appears exactly on the opposite side of the sun in the sky; it is the best time to observe a planet |
| Optical Doubles | Two stars at different distances that lie along nearly the same line of sight and thus appears close together |
| Perigee | The point in a satellite orbit when it is closest to the Earth |
| Perihelion | The point at which a body in an elliptical orbit around the sun is at its closest distance to the earth. |
| Planet | A large rocky or gaseous body that orbits a star |
| Planetary Nebula | A bright nebula thrown off by a dying star. |
| Precession | A 26,000 year wobbling cycle of the Earth's rotation axis that causes a gradual shift of the celestial poles and celestial coordinates |
| Pulsar | A celestial object that emits radio energy (sometimes light) in short, regular bursts; probably a rapidly rotating neutron star |
| Quasars | The extremely energetic early stage in the formation of an active galaxy, characterized by an output of radiation |
| RA | Abbreviation of Right Ascension which along with Declination defines a position in the sky. RA is measured eastward along the celestial equator with the zero point at the vernal equinox; it is specified in hours, minutes and seconds. |
| Reflection Nebula | A dust cloud reflecting starlight. |
| Reflector Telescope | A telescope that uses a curved mirror to gather light |
| Refractor Telescope | A telescope that uses a glass lens to gather light |
| Retrograde | The apparent reversal of the normal west to east motion of outer planets of outer planets as the Earth passes them |
| Right Ascension | The celestial equivalent to lines of longitude, which runs through the celestial poles and are perpendicular to the celestial equator; they are scaled in hours, increasing eastward from 0h and going full circle to 24h |
| Rotation | The spinning of a planet or other objects on its axis. |
| Sidereal Time | A time scale based on the true period of Earth's rotation; the time from star rise to star rise; 4 minutes shorter than the 24 hour day |
| Solar Eclipse | The passage of the moon's shadow across the earth |
| Solar System | The system containing the sun and all the smaller bodies in orbit around it |
| Spectrum | The array of colors or wavelengths that appears when light from an object is dispersed |
| Star | A self luminous sphere of hot gas held together by gravity; ordinary stars generate energy by nuclear fusion in their cores |
| Stellar Classification | Stars given a designation consisting of a letter and a number according to the nature of their spectral lines which corresponds roughly to surface temperature. The classes are O, B, A, F, G, K, and M. O Stars are the hottest; M the coolest. The numbers are simply subdivision of the major classes. The classes are oddly sequenced because they were assigned long ago before we understood their relationship to temperature. O and B stars are rare but very bright. M stars are numerous but dim. Our sun is designated G2. |
| Sunspot | A relatively cool dark area where magnetic fields piece the solar surface |
| Supergiant Star | Only the most massive stars become supergiants, after passing through the giant stage |
| Superior Conjunction | The place in which a planet whose orbit is inside that of the Earth, passes on the far side of the Sun with respect to the Earth |
| Supernova | An unusually violent explosion of a star which results in an increase in brightness of hundreds of millions of times. |
| Supernova Remnant | Leftover gas from a supernova explosion. |
| Variable Star | A star whose apparent brightness changes over time |
| White Dwarf | A small dense hot white star; the final stage in the evolution of stars with masses similar to the sun's or smaller |
| Young | Young for a star must be interpreted in the context of the average stellar lifetime of billions of years. A young star is one that is no more than a few million years old. |
| Zenith | The point in the sky directly over an observer's head |
| Sun | Alluding to our own Sun; sun and star are interchangeable |
| Parsec | Equal to 3-1/4 Light Years |
| Horizon | Imaginary horizontal line lying at eye level in all directions from you; 90 degrees from the zenith |
| Energy | Parts of the spectrum detectable only by instruments; i.e., X-rays, infrared, microwave, etc. |
| Airglow | The sky's natural fluorescence. It's caused by the sun's invisible but powerful ultraviolet radiation, which excites our atmosphere's gases to glow like the hand of a luminous watch |
| Event Horizon | The boundary of a black hole where space and time curve back unto themselves. |
| Singularity | The black hole's center where an entire star weighing 2 million planet Earths has been crushed down to less than the size of an atom |
| White Hole | Suggested by Einstein and mathematician Nathan Rosen that a tunnel, a wormhole, could provide a conduit for the black hole and its contents to reemerge in another place or time |
| Hubble Flow | One of the names for the expansion of the universe |
| Earthshine | The crescent moons dark unlit portion glows; traditionally called "the old moon in the new moon's arms". A portrait of our own planet's light reflected back to our eyes |
| Ashen Light | An enveloping halo that spills around the planet Venus to produce a complete ring when the crescent is very thin |
| Planesphere | A wheel like device displaying the orientation of the stars on any chosen date and time |
| Association | Family members of stars forming a large and unconfined cluster |
| Junkosphere | Space garbage producing a girdle of scrap metal surround our world |
| Meteoroids | Tine, nonglowing chunks of stone and metal out in space |
| Crepuscular Rays | During a sunset, bright pinkish streams will appear if the air si dusty or humid with distant cumulus clouds |
| Antisolar Rays | In some parts of the world, crepuscular rays often cross the sky to meet at the point opposite the sun |
| Time Dilation | According to Einstein's special relativity theory, time warps and slows on its own |
| Moon Illusion | Perhaps the most powerful mirage of all, the moon seems enormous when down near the horizon, a visual effect caused by its proximity to foreground terrestrial objects |
| Maunder Minimum | The period of 1640 to 1710 where the total loss of the sunspot cycle on the sun created a period of extraordinary cold |