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B & W Chapter 21
Stars, Galaxies, and the Universe
Question | Answer |
---|---|
TELESCOPE | A DEVICE BUILT TO OBSERVE DISTANT OBJECTS BY MAKING THEM APPEAR CLOSER |
VISIBLE LIGHT | ELECTROMAGNETIC WAVES THAT ARE VISIBLE TO THE HUMAN EYE |
WAVELENGTH | THE DISTANCE BETWEEN THE CREST OF ONE WAVE TO THE CREST OF THE NEXT WAVE |
SPECTRUM | THE RANGE OF WAVELENGTHS OF ELECTROMAGNETIC WAVES |
OPTICAL TELESCOPE | A TELESCOPE THAT USES LENSES OR MIRRORS TO COLLECT AND FOCUS VISIBLE LIGHT |
ELECTROMAGNETIC RADIATION | THE ENERGY TRANSFERRED THROUGH SPACE BY ELECTROMAGNETIC WAVES |
REFRACTING TELESCOPE | A TELESCOPE THAT USES CONVEX LENSES TO GATHER AND FOCUS LIGHT |
CONVEX LENS | A PIECE OF TRANSPARENT GLASS CURVED SO THAT THE MIDDLE IS THICKER THAN THE EDGES |
REFLECTING TELESCOPE | A TELESCOPE THAT USES A CURVED MIRROR TO COLLECT AND FOCUS LIGHT |
RADIO TELESCOPE | A DEVICE USED TO DETECT RADIO WAVES FROM OBJECTS IN SPACE |
OBSERVATORY | A BUILDING THAT CONTAINS ONE OR MORE TELESCOPES |
CONSTELLATION | AN IMAGINARY PATTERN OF STARS IN THE SKY |
SPECTROGRAPH | AN INSTRUMENT THAT SEPARATES LIGHT INTO COLORS AND MAKES AN IMAGE OF THE RESULTING SPECTRUM |
APPARENT BRIGHTNESS | THE BRIGHTNESS OF A STAR AS SEEN FROM EARTH |
ABSOLUTE BRIGHTNESS | THE BRIGHTNESS A STAR WOULD HAVE IF IT WERE A STANDARD DISTANCE FROM EARTH |
LIGHT-YEAR | THE DISTANCE LIGHT TRAVELS IN ONE YEAR |
PARALLAX | THE APPARENT CHANGE IN POSITION OF AN OBJECT WHEN SEEN FROM DIFFERENT PLACES |
HERTZSPRUNG-RUSSELL DIAGRAM | A GRAPH RELATING THE SURFACE TEMPERATURES AND ABSOLUTE BRIGHTNESSES OF STARS |
MAIN SEQUENCE | A DIAGONAL AREA ON AN H-R DIAGRAM THAT INCLUDES MORE THAN 90% OF ALL STARS |
NEBULA | THE CLOUD-LIKE REGION OF GASES LEFT OVER IN THE REMAINS OF A SHRINKING, SUN-SIZED STAR |
PROTOSTAR | A CONTRACTING CLOUD OF GAS AND DUST WITH ENOUGH MASS TO FORM A STAR |
WHITE DWARF | THE BLUE-WHITE HOT CORE OF A STAR THAT IS LEFT BEHIND AFTER ITS OUTER LAYERS HAVE EXPANDED AND DRIFTED OUT INTO SPACE |
SUPERNOVA | AN EXPLOSION OF A MASSIVE STAR |
NEUTRON STAR | THE SMALL, DENSE REMAINS OF A HIGH-MASS STAR AFTER A SUPERNOVA |
PULSAR | A RAPIDLY SPINNING NEUTRON STAR THAT PRODUCES RADIO WAVES |
BLACK HOLE | AN OBJECT WHOSE GRAVITY IS SO STRONG THAT NOTHING, NOT EVEN LIGHT, CAN ESCAPE |
BINARY STAR | A STAR SYSTEM WITH TWO STARS |
ECLIPSING BINARY | A BINARY STAR SYSTEM IN WHICH ONE STAR PERIODICALLY BLOCKS THE LIGHT FROM THE OTHER |
OPEN CLUSTER | A STAR CLUSTER THAT HAS A LOOSE, DISORGANIZED APPEARANCE AND CONTAINS NO MORE THAN A FEW THOUSAND STARS |
GLOBULAR CLUSTER | A LARGE, ROUND, DENSELY-PACKED GROUPING OF OLDER STARS |
GALAXY | A HUGE GROUP OF SINGLE STARS, STAR SYSTEMS, STAR CLUSTERS, DUST, AND GAS BOUND TOGETHER BY GRAVITY |
SPIRAL GALAXY | A GALAXY WITH A BULGE IN THE MIDDLE AND ARMS THAT SPIRAL OUTWARD IN A PINWHEEL PATTERN |
ELLIPTICAL GALAXY | A GALAXY SHAPED LIKE A ROUND OR FLATTENED BALL, GENERALLY CONTAINING ONLY OLD STARS |
IRREGULAR GALAXY | A GALAXY THAT DOES NOT HAVE A REGULAR SHAPE |
QUASAR | AN ENORMOUSLY BRIGHT, DISTANT GALAXY WITH A GIANT BLACK HOLE AT ITS CENTER |
UNIVERSE | ALL OF SPACE AND EVERYTHING IN IT |
SCIENTIFIC NOTATION | A MATHEMATICAL METHOD OF WRITING NUMBERS USING POWERS OF TEN |
BIG BANG | THE INITIAL EXPLOSION THAT RESULTED IN THE FORMATION AND EXPANSION OF THE UNIVERSE |
HUBBLE'S LAW | THE OBSERVATION THAT THE FARTHER AWAY A GALAXY IS, THE FASTER IT IS MOVING AWAY |
COSMIC BACKGROUND RADIATION | THE ELECTROMAGNETIC RADIATION LEFT OVER FROM THE BIG BANG |
SOLAR NEBULA | A LARGE CLOUD OF GAS AND DUST, SUCH AS THE ONE THAT FORMED OUR SOLAR SYSTEM |
PLANETESIMAL | ONE OF THE SMALL ASTEROID-LIKE BODIES THAT FORMED THE BUILDING BLOCKS OF THE PLANET |
DARK MATTER | MATTER THAT DOES NOT GIVE OFF ELECTROMAGNETIC RADIATION BUT IS QUITE ABUNDANT IN THE UNIVERSE |
DARK ENERGY | A MYSTERIOUS FORCE THAT APPEARS TO BE CAUSING THE EXPANSION OF THE UNIVERSE TO ACCELERATE |