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Group of stars that forms a pattern in the sky that looks like a familiar object, animal, or character |
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Measure of the amount of light a star actually gives off |
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Measure of the amount of light from a star that is received on Earth |
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The distance that light travels in one year |
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Lowest layer of the Sun's atmosphere; gives off light and has temperatures of about 6,000K |
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Layer of the Sun's atmosphere above the photoshere |
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Outermost, largest layer of the Sun's atmosphere; extends millions of kilometers into space and has temperatures up to 2,000,000K |
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Areas on the Sun's surface that are cooler and less bright than surrounding areas, are caused by the Sun's magnetic field, and occur in cycles |
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Late stage in the life cycle of comaratively low-mass main sequence star in which hydrogen in the core is deleted, the core contracts and temperatures inside the star increase, causing its outer layers to expand and cool |
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Late stage in the life cycle of comaratively low-mass main sequence star; formed when its core depletes its helium and its outer layers escape into space, leaving behind a hot dense core |
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Late stage in the life cycle of a massive star in which the core heats up, heavy elements form by fusion, and the star expands; can eventually explode to form a supernova |
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Collapsed core of a supernova that can shrink about 20km in diameter and conains only neutrons in the dense core |
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Final stage in the evolution of a very massive star, where the core's mass collapses to a point that its gravity is so strong that not even light can escape |
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Large group of stars, dust, and gas held together by gravity; can be elliptical, spiral, or irregular |
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States that about 13.7 billion years ago, the universe began with a huge, fiery explosion |
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Large cloud of gas and dust that contracts under gravitational force and breaks apart into smaller pieces, each of which might collapse to form a star |
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CME (coronal mass ejections) |
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Large ejections of electrically charged gas |
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How can the Sun be classified? |
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The sun can be classified as an average star |
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How is the energy of the Sun produced? |
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The Sun produces its energy by combining hydrogen into helium in its core |
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How does our Sun differ from most other main sequence stars? |
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Our Sun is the closest to Earth |
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How long is a light year? |
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9.5 trillion kilometers long |
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How far is Proxima Centauri from our solar syatem? |
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How do CMEs affect Earth? |
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How are sunspots related to prominences and solar flares? |
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Sunspots cause solar flares and prominences because sunspots have intense magnetic fields |
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True or Faulse; the Sun is a main sequence star |
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True or Faulse; Polaris is in Ursa Major |
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What are the three types of galaxys? |
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Spiral, elliptical, or irregular |
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