asro ch 1 – Space – Flashcards

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186,000 miles per second
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speed of light
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the distances to bodies in the solar system are a few light minutes to light hours
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true
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it was aristotle who used the scientific method to show the earth was a sphere
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true
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constellations are close clusters of stars, all at about the same distance from the sun
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false
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from the south pole Polaris would appear directly overhead
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false
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only at the equator are all the stars visible over the course of the year
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true
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over the course of a night Polaris moves less than any other visible star in the sky
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true
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there are 3,600 arc seconds in a degree
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true
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a star with a right ascension of 2.6 hours will rise 2.6 hours after the vernal equinox
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true
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in general the brightest star in a given constellation is designated as alpha
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true
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the south celestial pole is located at a declination of -90 degrees
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true
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at apogee the moon is at its farthest from earth and thus appears smaller than normal because of this it can produce only annular solar eclipses, but not total solar eclipses.
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true
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The blocking of sunlight to the moon that occurs when Earth is directly between the sun and the moon.
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lunar eclipse
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occurs when the Moon passes directly between the Sun and Earth and casts a shadow over part of Earth
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solar eclipse
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from earth, the sun and moon have about the same angular diameter
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true
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the full moon rises at sunrise and sets at sunset
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false
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from full moon to third quarter moon takes about a week.
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true
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the first quarter moon will rise about noon and set about midnight
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true
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as it orbits the earth , the moon appears to move eastward about its own diameter every hour
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true
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the parallax shift of a star would be greater if viewed from mars than from earth
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true
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an apparent shift in the position of an object when viewed from different locations
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parallax
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totality of all space, time, matter, and energy
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universe
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study of the universe
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Astronomy
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the distance light travels in a years
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about 10 trillion miles
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these must be : Must be testable • Must be continually tested • Should be simple • Should be elegant
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scientific theories
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observation leads to __- in the scientific method which then leads to ___
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theory, predictions
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how many stars are visible at any one time? at any one time
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3000 stars
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Figures having meaning to those doing the grouping
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constellations
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invisible sphere that surrounds our earth that shows the locations of constellations, Is useful for locating objects in the sky.Stars seem to be on the inner surface of a sphere surrounding the Earth They aren't, but can use two-dimensional spherical coordinates (similar to latitude and longitude) to locate sky objects
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The celestial sphere
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a full circle contains _____ degrees. each degree contains ___ arc minutes each arc minute contains ____arc seconds
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360, 60′, 60′′
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Seasonal changes to night sky are due to ________________
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Earth's motion around Sun
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Twelve constellations Sun moves through during the year are called the ______, path is ecliptic
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zodiac
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• Combination of ______ and ________ gives seasons
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day length , sunlight angle
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• Northernmost point of path (above celestial equator) is calledd the ____________, Day with the most hours of sunlight and the fewest hours of darkness
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summer solstice
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southernmost point of path is called the ________, Occurs when the Sun is directly overhead at 23.5° south latitude, around December 21, and results in the minimum number of daylight hours for the northern hemisphere and the maximum number for the southern hemisphere.
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winter solstice
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points where path crosses celestial equator are called the _____ and the ____________, Earth's axis of rotation is perpendicular to the line joining Earth to the Sun, so day and night are equal length
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vernal and autumnal equinoxes
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Time from one vernal equinox to next is ______
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tropical year
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rotation of Earth's axis itself; makes one complete circle in about 26,000 years
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Precession
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Time for Earth to orbit once around Sun, relative to fixed stars, is ________, , the time required for Earth to complete one orbit around the Sun, relative to the stars
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sidereal year
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Tropical year follows ________; sidereal year follows ________
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seasons, constellations
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Moon takes about ________days to go through whole cycle of phases called a ____________.
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29.5 , synodic month
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moon ______ are due to different amounts of sunlit portion being visible from Earth
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phases
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Time to make full 360° rotation around Earth,is about 2 days shorter, The average period of revolution of the Moon around the Earth in reference to a fixed star, equal to 27 days, 7 hours, 43 minutes in units of mean solar time.
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sidereal month
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a sidereal month is about __________ days shorter
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2
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Eclipses don't occur every month because Earth's and Moon's orbits are not in the ________
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same plane
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Measure baseline and angles, can calculate distance, a trigonometric method of determining the position of a fixed point from the angles to it from two fixed points a known distance apart
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Triangulation
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the period of time from which the sun is directly overhead until the next time the sun is directly overhead., From noontime to the next noontime; for Earth it is 24 hours.
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solar day
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The period of revolution of the Moon with respect to the Sun; the length of one cycle of lunar phases; 29 1/2 Earth days., The period of revolution of the Moon with respect to the Sun; the length of one cycle of lunar phases. Also called the lunar month.
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Synodic month
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Distances can be measured through ________ and ___________
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triangulation and parallax
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Tropical year ≠ sidereal year, due to ____ of Earth's axis
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precession
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Synodic month ≠ sidereal month, also due to earths ______ around sun
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rotation
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Solar day ≠ sidereal day, due to Earth's _____ around sun.
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rotation
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• Angle of Earth's axis causes _____
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seasons
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Moon shines by reflected light, has ___
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phases
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Plane of Earth's orbit around Sun is ___- at ____ degrees to celestial equator
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ecliptic, 23.5
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Measuring Earth's radius: Done by _______ about 2300 years ago; noticed that when Sun was directly overhead in one city, it was at an _____in another
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Eratosthenes , angle
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a slow motion of Earth's axis that traces out a cone over a period of 26,000 years
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precession
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