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ESPS
Science
| Question | Answer |
|---|---|
| Astronomy, | the branch of science that deals with celestial objects, space, and the physical universe as a whole. |
| Big Bang Theory, | a theory in astronomy: the universe originated billions of years ago in an explosion from a single point of nearly infinite energy density — compare steady state theory. |
| Doppler Shift | a change in frequency due to the Doppler effect. |
| , Red Shift, | the displacement of spectral lines toward longer wavelengths (the red end of the spectrum) in radiation from distant galaxies and celestial objects. |
| Blue Shift, | the displacement of the spectrum to shorter wavelengths in the light coming from distant celestial objects moving toward the observer. |
| , Red giant, | a very large star of high luminosity and low surface temperature. Red giants are thought to be in a late stage of evolution when no hydrogen remains in the core to fuel nuclear fusion. |
| Frequency, | the rate at which something occurs or is repeated over a particular period of time or in a given sample. |
| White dwarf, | a small very dense star that is typically the size of a planet. A white dwarf is formed when a low-mass star has exhausted all its central nuclear fuel and lost its outer layers as a planetary nebula. |
| Nova | a star showing a sudden large increase in brightness and then slowly returning to its original state over a few months. |
| , Neutron star, | a celestial object of very small radius (typically 18 miles/30 km) and very high density, composed predominantly of closely packed neutrons. |
| Pulsar, | a celestial object, thought to be a rapidly rotating neutron star, that emits regular pulses of radio waves and other electromagnetic radiation at rates of up to one thousand pulses per second. |
| Black Hole, | a region of space having a gravitational field so intense that no matter or radiation can escape. |
| Constellations, | a group of stars forming a recognizable pattern that is traditionally named after its apparent form or identified with a mythological figure. |
| Absolute Brightness (magnitude), | the measure of intrinsic brightness of a celestial object. It is the hypothetical apparent magnitude of an object at a standard distance of exactly 10 parsecs (32.6 light years) from the observer, assuming no astronomical extinction of starlight. |
| Apparent Brightness (magnitude), | The brighter an object appears, the lower its magnitude value (i.e. inverse relation). |
| Cosmic Microwave Background, | thermal radiation left over from the time of recombination in Big Bang cosmology |
| Universe, | all existing matter and space considered as a whole; the cosmos |
| Galaxy , | a system of millions or billions of stars, together with gas and dust, held together by gravitational attraction. |
| Solar System, | the collection of eight planets and their moons in orbit around the sun, together with smaller bodies in the form of asteroids, meteoroids, and comets. |
| Star | . a fixed luminous point in the night sky that is a large, remote incandescent body like the sun. |
| Electromagnetic Spectrum, | the range of wavelengths or frequencies over which electromagnetic radiation extends. |
| AU- Astronomical Unit, | is a unit of length, roughly the distance from Earth to the Sun. |
| Solar Nebula, | describes the formation of our solar system from a nebula cloud made from a collection of dust and gas. It is believed that the sun, planets, moons, and asteroids were formed around the same time around 4.5 billion years ago from a nebula. |
| Gas giant , | a large planet of relatively low density consisting predominantly of hydrogen and helium, such as Jupiter, Saturn, Uranus, or Neptune. |
| Nuclear fusion, | a nuclear reaction in which atomic nuclei of low atomic number fuse to form a heavier nucleus with the release of energy. |
| Convective zone | region of turbulent plasma between a star's core and its visible photosphere at the surface, through which energy is transferred by convection. |
| , Photosphere | the luminous envelope of a star from which its light and heat radiate. |