Term
| Kirchhoff's Laws of Radiation
Law 1: Continuous Spectrum |
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Definition
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radiate at all wavelengths and thus produce a continuous spectrum.
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Term
| Kirchhoffs Laws of Radiation
Law 2: Emission Spectrum |
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Definition
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a low-density gas excited to emit light will do so at specific wavelengths
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Term
| Kirchhoff's Laws of Radiation
Law 3: Absorption Spectrum |
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Definition
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if light with continuous spectrum passes through a cool, low-density gas which absorbs them, it will produce an absorption spectrum.
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Term
| The only thing that radiates a continuous spectrum (white light) |
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Definition
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Term
| The one thing you need to know about a black body |
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Definition
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Term
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Definition
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motion of an object causes the wavelength to change; motion toward the observer shifts the color blue, and vice versa for red.
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Term
| Temperature sequence classifications for stars |
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Definition
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OBAFGKM, 0-9, 0 being the hottest and so forth.
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Definition
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Term
| Hertzprung-Russel (H-R) Diagram |
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Definition
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star's luminosity versus the Temperature/spectral type; stars are found in specific regions of the diagram. 90% of stars fall on the Main Sequence line.
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dying stars, high T/low L
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Term
| few electrons make it to n=2 state |
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Definition
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Definition
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everything but hydrogen/helium...the others are easier to move electrons, since the outer ones are weakly bound.
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Definition
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both stars seen in telescope, gravitational pull to each other.
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Definition
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Doppler shift, only one star visible; SB1-one set of shifting lines...SB2=two
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Term
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Definition
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Winking Star (demon Star)
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Term
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Definition
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Interstellar Medium; mostly made of hydrogen (75%) and helium (25%)
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Term
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Definition
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luminous clouds typically red in color, associated with O or B type stars.
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Definition
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Opaque, made mostly of dust grains and complex molecules....also known as Molecular clouds.
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Term
| Dark clouds are gravitationally stable when... |
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Definition
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outward gas pressure= inward gravitational force...they need something to initiate the cloud collapse, such as a shock wave
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Definition
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supernova explosions, spiral arms in galaxies, collisions between clouds, between galaxies....
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Definition
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the beginning of the forming of a star, as it starts to collapse in on itself.
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Definition
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small dark clouds in emission nebulae, possible sites of collapsing clouds.
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Term
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Definition
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As cloud collapses, sun condenses in the middle, with a ring/disk of matter around it, creating planets.
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Term
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Definition
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without H and He, formed in high T region of Solar nebula.
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Term
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Definition
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low density, large in size, many moons and often ring systems; large atmospheres
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Definition
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star forms in core, disk forms because of angular momentum.
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Definition
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converting four H into one He, mass loss.
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Definition
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heat transfer dominated by photons (heat from fire/sun
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Definition
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energy transport dominated by gas motion (boiling pot of water)
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Definition
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energy transport by contact (heat transferred along a metal spoon)
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Definition
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region where photons escape the sun; Granules=convection cells, about the size of Texas.
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Definition
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typical size of an atom; optical light= 4000A-7000A
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Definition
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found temperature sequence in Anni Jump Cannon's spectral classification.
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