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telescopes and Oceans Games

AB
seafloormany of the same features as land, higher mountains, extensive plains, deeper canyons
continental shelfsloping part of the continent that is covered with water from its shoreline to the continental slope
continental slopesteeply sloping area that connects the continental shelf and the deep ocean floor
continental risegently sloping surace at the base of the continental slope
abyssal plainsflat, level parts of the ocean floor
seamountundersea volcano peak that is at least 1000 meters avove the ocean floor
guyota submerged flat-topped seamount
mid ocean ridgesare continuous undersea mountain chains found in the middle of the oceans
ocean trencheslong,narrow trouchs or depressions formed where ocean floors collide with another section of ocean floor or continent
Marianas Trenchll km deep, deepest trench in the Pacific Ocean
submerged shorelinesea has risen or land has shrunk
hydrospherecovers 70 percent of the earth's surface that is covered in salt water (mass 1.4 X 10 to 24th power grams)
Oceans7 North Atlantic, South Atlantic, North Pacific, South Pacific, Indian, Arctic, Antarctic
Salinitynumber of grams of these dissolved salts in 1000 grams of sea water (3.5%) salt being most abundant (low near river mouths and high in areas of high evaporation rates)
Ocean temperatureconstant to depths of 90 meters (28 degrees C at equator to 2 degrees C at poles) Freezing point of seawater is lower than freezing point of pure water) Freezing point varies with the salinity of the water (-2 C to 0C)
Temperature zones of the oceanSurface layer, mixed area- called thermocline (wind and waves churn where living creatures live) and third layer that is cold dark to barren ocean floor
oozesname given to the sediment that contains at least 30% plant or animal shell fragments -contains calcium carbonate
authigenic depositsdeposits formed directly from sea water
seamountsunderwater wolcanoes-magna rising from the hot spot punches through the plate and forms a volcano - Hawaiian islands
Lateriteswet and tropical, red-orange soil rich in iron and aluminum oxides little humus soil not very fertile
refracting telescopeuses lenses to bend light rays in focusing the image (Galilee)
reflecting telescopeuses mirrors to gather light rays on a curved mirror which produced image (Newton)
Hubble Space telescopeuses a single relector mirror. It observes objects seven times farther away
optical telescopesrefracting and reflecting telescopes since they gather visible light and focus it to produce an image
radio telescopecollects invisible radio waves created by the sun and stars- It has a reflector or dish with special receivers (advantages- receive 24 hrs a day, operate in any kind of weather, ability to detect objects from great distances in space) largest in Puerto Rico dish more than 300 meters in diameter)
spectroscopedevice attached to telescopes used to separate white light into a series different color by wave lengths called a spectrum (used to observe spectra, temperatures, pressures, and movement of stars)
spectographphotographs a spectrum (red longest wavelength, violet the shortest)
electromagnetic spectrumarrangement of wavelengths- range from very long radio waves to very short gamma rays
Star moving toward earthlight waves compress and wavelenghs are shorter so moves toward blue or violet
Star is moving away from earthlight waves expand and wavelengths seem longer. moves toward the red end of the spectrum
AU or astronomical unitthe distance from the earth to the sun (150 X 10 to the sixth power)- used to measure distances within our solar system
LY or light yearthe distance light travels in one year or 9.5 X 10 to the twelth power - used to measure distances in space
parsecmeasures large distances in space =a distance of 3.26 light years
Planets in our solar systemMercury Venus Earth Mars (inner planets) Jupiter Saturn Uranus Neptune and Pluto (outer planets)
Mercuryclosest planet to the sun, craters and rocks, hydrogen, helium and sodium in the atmosphere (named after Roman messenger god)
Venusslow rotation , rotates opposite the earth (retrograde rotation), extensive cloud coverage so cannot see surface, atmosphere mostly carbon dioxide, clouds contain sulfuric acid giving a yellow appearance, clouds trap heat (named Roman goddess of love)
Eartha water planet, gravity holds water in place, different temperatures on earth allow water to exist as a solid, liquid and gas. Atmosphere is mostly oxygen and nitrogen, only planet known to support life
Marsnumerous craters, active and extinct volcanoes, ridges and valleys, iron oxide in soil giving rust color to surface, atmosphere has carbon dioxide, nitrogen, argon oxygen and water vapor, polar ice caps of water, two satellites (named after Roman war god)
Jupiterlargest planet, 16 moons, atmosphere of hydrogen, helium, methane, and ammonia, rising and and descending gases caused by heat from the core, Great Red Spot thought to be hurricane cloud, strong magnetic field
Saturnseond largest planet, rings of ice and rock and dust particles, stmosphere of hydrogen, helium, methane, and ammonia, 20+ satelites (named after Roman god of agriculture)
Uranusretrograde (reverse) rotation, gaseous planet, 10 dark rings and 15 satellites, atmosphere is hydrogen, helium, and methane (named after Greek god of the heavens)
Neptunegaseous planet, atmosphere of hydrogen, helium and methane, 3 rings and 2 satellites,(named after Roman sea god, atmosphere has the color of the seas)
Plutosmallest planet, atmosphere thought to contain methane, ammonia, and frozen water, 1 satellite, revolves around the sun every 250 years (named after Roman god of the underworld)
Asteroidsfound in the region between Mars and Jupiter
Cometsmasses of frozen gases, cosmic dust, and small rocky particles, think they originate in a comet cloud beyond Pluto- it has a nucleus, a coma, and a tail, The tail points away from the sun
Halley's cometdiscovered in 240 BC it returns every 75 to 76 years
Meteoroidscomposed of particles of rock and metal, it burns in our atmosphere and then called a meteor or a shooting star
Meteoritesmeteors that strike the earth's surface, Barringer Crater in Arizone
constellationspatterns of stars as a reference to locate other stars
Ursa Majorbig bear constellation
Ursa Minorlittle bear constellation
The Big Dipperfound within the Ursa Major
The Little Dipperfound within Ursa Minor
Magnitude stars21 of the brightest stars seen from earth
galaxiesVast collection of stars
irregular galaxyno real structed appearance, early stage of life
elliptical galaxysmooth ellipses containing little dust and gas composed of millions and millions of stars
spiral galaxydisk shaped with extended arms that rotate around a dense center, earth is in the Milky Way Galaxy and it is a spiral galaxy
pulsarvariable radio source that emits signals in very short regular bursts, it is believed to bea rotating neutron star
quasarobject that photographs like a star but has an extremely large redshift and a variable energy output, believed to be the active core of a very distant galaxy
black holesobject that has collapsed to such a degree that light can not escape from its surface, light is trapped by the intense gravitational field
BlueshiftThe shortening of a light wave from an object moving toward an observer. For example, when a star is traveling toward Earth, its light appears bluer.
ComaThe cloud of gas and dust that forms around a comet's nucleus. This cloud is created when the solar wind strikes the surface of the nucleus.
CoronaThe outermost layer of the atmosphere of a star, including the Sun. The corona is visible during a solar eclipse or when special adapters or filters are attached to a telescope to block the light from the star’s central region. The gaseous corona extends millions of kilometers from the star’s surface and has a temperature in the millions of degrees.
InfraredRadiation that has longer wavelengths and lower frequencies and energies than visible light.
ParallaxThe apparent shift of an object’s position when viewed from different locations. Parallax, also called trigonometric parallax, is used to determine the distance to nearby stars. As the Earth’s position changes during its yearly orbit around the Sun, the apparent locations of nearby stars slightly shift. The stars’ distances can be calculated from those slight shifts with basic trigonometric methods.


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