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astro flashcards

Ethan Reid Physics English 56 cards

astro flashcards

Cards in this deck (56)

  1. 1Kepler's First LawThe orbit of each planet around the Sun is an ellipse with the Sun at one focus.
  2. 2Kepler's Second LawAs a planet moves around its orbit, it sweeps out equal areas in equal times
  3. 3Kepler's Third Law (in words)The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
  4. 4Kepler's Third Law (Newton's formula)Kepler's Third Law (Newton's formula)
  5. 5Escape velocity (formula)Escape velocity (formula)
  6. 6Parallax equation with baselineParallax equation with baseline
  7. 7Impact crater equationImpact crater equation
  8. 8Flux recieved from sun at distance dFlux recieved from sun at distance d
  9. 9Power absorption of a planetPower absorption of a planet
  10. 10Thermal equilibrium of planet predictionThermal equilibrium of planet prediction
  11. 11Relationship between cooling time and radius of planetRelationship between cooling time and radius of planet
  12. 12Roche LimitRoche Limit
  13. 13Classical doppler shiftClassical doppler shift
  14. 14Radius of a planet in transitRadius of a planet in transit
  15. 15Kepler's Third Law (reduced formula)Kepler's Third Law (reduced formula)
  16. 16Earth-like criterionmass < 2 earth masses
  17. 17Super earth criterion (and significance)mass between 2 and 10 earth masses (at 10 earth masses the planet is large enough to become a gas giant)
  18. 18Neptune-like criterionmass between 10 Earth masses and 2 Neptune masses
  19. 19Jupiter-like criterionmass greater than 2 Neptune masses
  20. 20hot planet criteriondistance from star less than 0.1AU
  21. 21cold planet criteriondistance from star greater than 1AU
  22. 22criteria for magnetosphere to form1. Liquid core
    2. Core is made of ferromagnetic material (or metallic hydrogen)
    3. Rapid rotational speed
  23. 23composition of comets' tailion tail caused by solar wind +
    dust tail caused by dust escaping the coma
  24. 243 methods of exoplanetary search1. doppler shift measurement
    2. planetary transits
    3. direct imaging
  25. 25meteoroidsobjects with potential to hit Earth
  26. 26meteorsthe flash of light produced when a meteoroid enters the atmosphere and encounters frictional heating
  27. 27meteoritesremnants of meteoroids that have made it to the surface
  28. 28when do meteor showers occurwhen Earth passes through cometary debris, occuring periodically
  29. 29range of Kupier belt30AU-500AU
  30. 30range of Oort cloud2000AU-100000AU
  31. 31L1 locationbetween the sun and earth: unstable
  32. 32L2 locationbetween Earth and Mars' orbit: unstable
  33. 33L3 locationdirectly opposite Earth behind the Sun: unstable
  34. 34L4 & L5 location60 degrees behind and in front of Earth's orbit, respectively: stable.
  35. 35range of asteroid belt2-3.5AU
  36. 36description of Iothe most volcanically active body within the solar system: caused by irregular orbit of Io and large tidal forces from Jupiter
  37. 37why is saturn hotter than expectedHelium rain falling generates frictional heat
  38. 38Why can rings be forced to be narrow by shepherd moonsif there is a satellite on both sides of the ring, the inner (outer) satellite causes a heating (cooling) effect resulting in higher (lower) orbits. this constricts the range of radii
  39. 39What is differential rotationWhen the angular velocity of a fluid body is not constant at all places, e.g. smaller rotational period at the equator
  40. 40Why are neptune and uranus bluedue to the methane in their upper atmosphere. more methane = more blue
  41. 41possible explanation for uranus and neptune's odd B fieldsfrozen ammonia dissolved into water acts as the conductive fluid for the dynamo effect. the fluid's currents are located far from the core then it could work
  42. 42which jovian planet has no internal heat sourceuranus
  43. 43why is neptune hotter than expectedmethane in atmosphere insulates heat (similar to greenhouse effect)
  44. 44why is jupiter hotter than expectedjupiter has a (relatively) large surface area to volume ratio, so it loses heat from its surface slower than the other planets
  45. 45why is there a discrepancy in expected heat in Earth and Venusthe greenhouse effect
  46. 46what is albedoalbedo is the fraction of power that is reflected by a planet's surface
  47. 47why does venus have retrograde motionlikely due to an early collision changing the direction of its rotation
  48. 48why is Earth's moon relatively largeit was likely created during the collision of a young, larger Earth with a mars-sized object. the debris began orbiting Earth and coalesced over time into the moon
  49. 49why was the copernical model shitit had to use the idea of epicycles in orbits to explain observations of the planets.
  50. 50Wien's LawWien's Law
  51. 51Power output of starPower output of star
  52. 52Measured flux from a star at distance DMeasured flux from a star at distance D
  53. 53wavelength of emitted photons in hydrogenwavelength of emitted photons in hydrogen
  54. 54rayleigh scattering proportionalityrayleigh scattering proportionality
  55. 55rayleigh criterionrayleigh criterion
  56. 56degrees to arc units conversion1 degree = 60 arcminutes
    1 arcminute = 60 arcseconds

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Physics Flashcards on astro flashcards, created by Ethan Reid on 25/04/2024.
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Ethan Reid
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