Astronomy Exam 2 Flashcards
Flux
Brightness
Wavelength
Color
The only directly measurable quantities in astronomy
Brightness, Color, Position, Time, Polarization (+ Particles)
Kirchhoff’s Rules
Rules governing the emission of radiation by heated gases and solids
Kirchhoff’s Rules #1
A hot, opaque gas or solid will glow with a continuous spectrum
Kirchhoff’s Rules #2
A hot transparent gas emits light only at specific wavelengths that depend of the composition of the gas. This an emission line spectrum
Kirchhoff’s Rules #3
A cool gas placed between the observer and a continuous spectrum source absorbs light at specific wavelengths that depend on the composition of the gas
Spectrum
A representation of the amount of light something emits at each color or “wavelength”
Light
Any kind of electromagnetic radiation, not just colors we can see with our eyes
Continuum Spectrum
The wavelength of the peak in the continuum spectrum grows shorter (bluer) for hotter substances
Every atom has a ________ spectrum
Different
Bluer Photons
Higher Energies
Redder Photons
Lower Energies
When electron absorbs energy from a photon, it moves out to _____ orbital level
Higher
The greatest jump means the ________ the most energy
absorbing
Planet means
Wanderer
Pluto was considered a planet between
1930-2006
8 Planets
Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune
Definition of Planet
A celestial body that is in orbit around the sun, has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and has cleared the neighborhood around its orbit.
Definition of Dwarf Planet
A celestial body that is in orbit around the sun and has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape
Solar System Properties
Terrestrial (rocky) is close to the sun, Jovian (gaseous) planets are farther away.
Orbits all lie in the same place, orbit in the same direction.
Most of the stuff (mass) in the sun.
Astrometry
Precisely measuring the positions of the stars in the sky
Transit
When one astronomical body appears to move across the face of another
Distance to closest star (besides the Sun)
4.2 light-years
Luminosity (L)
Total amount of power a star emits into space (does not depend on observing distance)
Flux (F)
Power per unit area; measures parent brightness (does depend on distance)
Distance (d)
Distance to emitting object (e.g., a star)