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ESPS Semester 1
| Term | Definition |
|---|---|
| Astronomy | The branch of science that deals with space, objects in space, and the physical universe as a whole. |
| Big Bang Theory | The theory that the universe may have been created in a huge explosion at least 12 billion years ago. |
| Doppler Shift | A change in the frequency of sound, light, or other waves. |
| Red Shift | A shift toward longer wavelengths of spectral lines emitted by an object in space that is caused by an object moving away from the earth. |
| Blue Shift | A shift toward shorter wavelengths of spectral lines of an object in space caused by the motion of the object toward the observer. |
| Frequency | The number of crests of a wave that move past a given point in a given unit of time. |
| Wavelength | The distance measured in the direction of a wave between two successive points. |
| Absolute Brightness | The brightness a star would have if it were placed at a distance of 10 parsecs from Earth. |
| Apparent Brightness | A number that is a measure of its brightness as seen by an observer on Earth. |
| Cosmic Microwave Background | Radiation coming from space that originated from the Big Bang. |
| Universe | The whole of all matter, energy, planets, galaxies, and space. |
| Galaxy | The system of millions or billions of stars together with gas and dust held by a gravitational attraction. |
| Solar System | The collection of eight planets and their moons in orbit around the sun with asteroids, meteoroids, and comets. |
| Star | A fixed luminous point in the sky. |
| Planet | A large object in space that orbits a star such as the sun and does not produce its own light. |
| Electromagnetic Spectrum | The range of wavelengths or frequencies where electromagnetic radiation extends. |
| AU-Astronomical Unit | The distance between Earth and our sun or the amount of distance in a light year. |
| Solar Nebula | A Nebula cloud made from a collection of dust and gas. |
| Gas Giant | A large planet of low density consisting of hydrogen and helium, such as Jupiter. |
| Nuclear Fusion | A Nuclear reaction in which atomic nuclei fuse to form a heavier nucleus. |
| Convective Zone | A region of plasma between a star's core and its visible photosphere. |
| Photosphere | The luminous envelope of a star where the light and heat radiate from. |
| Chromosphere | A reddish gaseous layer above the photosphere of a sun or star. |
| Corona | A gaseous envelope of the sun and other stars. |
| Sunspot | A spot or patch appearing on the sun's surface from time to time. |
| Prominence | An eruption of high-density gas from a solar chromosphere. |
| Solar Flare | A sudden eruption of intense high-energy radiation from the sun's surface. |
| Coronal mass ejection | The release of plasma and magnetic field from the solar corona. |
| Light year | The equal distance in length that light travels in one year. |
| Parallax | The angular displacement of a celestial object due to being observed from the Earth instead of the Sun. |
| Main Sequence | A continuous band of stars that appears on plots of stellar color versus brightness. |
| HR Diagram | A scatter plot of stars showing the relationship between the stars' absolute magnitudes. |
| Nebula | A cloud of gas and dust in outer space. |
| Red Giant | A luminous giant star of low or intermediate mass. |
| White Dwarf | A small very dense star that is typically the size of a planet. |
| Nova | A star that shows a large increase in brightness and then slowly returns to its original state. |
| Neutron Star | A small dense star that is a collapsed core of a giant star. |
| Pulsar | A celestial object the rapidly rotates a neutron star. |
| Black Hole | A region of space having such a strong gravitational field that no matter or radiation can escape. |
| Constellations | A group of stars forming a pattern that is named after an apparent form or a mythological creature. |
| Cosmology | The branch of Astronomy that involves the origin and evolution of the universe from the Big Bang Theory to today. |