Statistics for Cosmology Review Pt. 1

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General Stats

  • This quiz has been taken 21 times
    (19 since last reset)
  • The average score is 12 of 58

Answer Stats

HintAnswer% Correct
does the moon rotate?yes
60%
Speed of light (kilometers)300,000 km/s
47%
How many official constellations are there?88
40%
the original last month in the calendarFebruary
40%
Point above observer's headzenith
40%
Speed of light (miles)186,000 m/s
33%
degree of earth's tilt23.5
33%
length of a solar day24h
33%
Point below observer's feetnadir
33%
the apparent shifting of an object with respect to more distant objects because of the changing of the observer's perspectiveparallax
33%
"wandering stars"planets
33%
the wobble of the earth as it rotates like a topprecession
33%
the number of years it takes the north celestial pole to travel in a circle (precession)26,000
27%
What does an arcsecond measure?angles
27%
celestial latitudedeclination
27%
the path of the Sun among the fixed starsecliptic
27%
"equal nights"equinox
27%
celestial longituderight ascension
27%
the 12 constellations the Sun passes throughzodiac
27%
the distance from the Earth to the Sun1AU
20%
number of years it takes the vernal equinox to pass to a new zodiac constellation2000
20%
the number of days it takes the moon to line up again with the Sun2.2
20%
the number of days it takes the moon to revolve 360 degrees (also a sidereal period)27.3
20%
Halfway between the celestial poles, perpendicular to the axiscelestial equator
20%
circle which passes through the zenith and nadircelestial meridian
20%
Equation for finding speed of lightd=vt
20%
Where is the prime meridian?Grenwich
20%
what insolation (sunlight spreading over the earth) actually meansincoming solar radiation
20%
months when the Earth is closest (perihelion)/farthest (aphelion) from the SunJanuary/July
20%
imaginary sun which moves along the celestial equator rather than the ecliptic and which matches the average motion of the real sunmean sun
20%
intersection of the orbit plane of a celestial body with the plane of the eclipticnode
20%
area close to the sunperihelion
20%
number of degrees the sun travels in an hour15
13%
length of a sidereal day23h56m4s
13%
time from one new moon to the next (synodic month)29.5 days
13%
before the local meridianante meridian (AM)
13%
area farther away from the sunaphelion
13%
parallax equationd=1/pi
13%
time between successive transits of a celestial objectday
13%
types of arc (largest to smallest)degree, minute, second
13%
days of the week in Frenchdimanche, lundi, mardi, mercredi, jeudi, vendredi, samedi
13%
when crossing this from east to west add a day, and when crossing from west to east subtract a dayinternational date line (IDL)
13%
the angle measured westward along the celestial equator from the local meridian to the hour circle (meridian) of the objectLHA (local hour angle)
13%
local hour angle of the actual sun +12hrslocal apparent solar time (LAST)
13%
local hour angle of the mean sun +12hrslocal mean solar time (LMST)
13%
local hour angle of the vernal equinoxlocal sidereal time (LST)
13%
phases of the moonnew, waxing crescent, first quarter, waxing gibbous, full, waning gibbous, third quarter, waning crescent
13%
Points at both ends of the celestial rotation axisnorth and south celestial poles
13%
after or past the local meridianpost meridian (PM)
13%
original names of July and AugustQuintilis and Sextilis
13%
takes synodic, nodical and anomalistic periods into account to predict the recurrence of an eclipseSaros cycle
13%
system used for angular measurementsexagesimal system
13%
used by ancient peoples to establish calendarssolstice principle
13%
stellar distances to the nearest starsstellar parallax
13%
when the Sun is furthest above the celestial equator (2x)summer and winter solstices
13%
places where the sun appears at the zenith at noon on the first day of the summer/winterTropics of Cancer and Capricorn
13%
where the ecliptic crosses the celestial equator (2x)vernal and autumnal equinoxes
13%
locations of the moon during a solar eclipsenew moon, moon at or near a node
0%

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