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93 Cards in this Set

  • Front
  • Back
total solar eclipse
a solar eclipse during which the Sun becomes fully blocked by the disk of the Moon
focus (of an ellipse)
one of two special points within an ellipse that lie along the major axis; when one object orbits a second object, the second object lies at one focus of the orbit
arcseconds
one arcsecond is 1/60 of an arcminute
analemma
the figure eight path traced by the Sun over the course of a year when viewed at the same place and the same time each day; represents the discrepancies between apparent and mean solar time
north celestial pole
the point on the celestial sphere directly above the Earth's North Pole
science
the search for knowledge that can be used to explain or predict natural phenomena in a way that can be confirmed by rigorous observations or experiments
constellation
a region of the sky
scientific theory
a model of some aspect of nature that has been rigorously tested and has passed all tests to date
pseudoscience
something that purports to be science or may appear to be scientific but does not adhere to the testing and verification requirements of the scientific method
lunar phase
describes the appearance of the Moon as seen from Earth
longitude
the angular east-west distance between the prime meridian and a location on the Earth's surface
annular solar eclipse
a solar eclipse during which the Moon is directly in front of the Sun but its angular size is not large enough to fully block the Sun; thus a ring (or annulus) of sunlight is still visible around the Moon's disk
meridian
a half-circle extending from your horizon due south, through your zenith, to your horizon due north
eclipse seasons
periods during which lunar and solar eclipses can occur because the modes of the Moon's orbit are nearly aligned with the Earth and Sun
antimatter
refers to any particle with the same mass as a particle of ordinary matter but whose other basic properties are precisely opposite
DNA
the molecule that represents the genetic material of life on Earth
precession
the gradual wobble of the axis of a rotating object around a vertical line
aphelion
the point at which an object orbiting the Sun is farthest from the Sun
altitude (above horizon)
the angular distance between the horizon and an object in the sky
Arctic Circle
the circle on the Earth with latitude 66.5 degrees N
winter solstice
the point on the celestial sphere where the ecliptic is farthest south of the celestial equator; the moment in time when the Sun appears at that point each year (December 21)
Ptolemaic model
the geocentric model of the universe developed by Ptolemy in about 150 AD
axis tilt
the amount by which a planet's axis is tilted with respect to a line perpendicular to the ecliptic plane
Copernican revolution
the dramatic change that occurred when we learned that Earth is a planet orbiting the Sun rather than the center of the universe
carbon dioxide cycle
the process that cycles carbon dioxide between the Earth's atmosphere and surface rocks
arcminutes
one arcminute is 1/60 of a degree
geocentric model
any of the ancient Greek models that were used to predict planetary positions under the assumption that Earth lay in the center of the universe
paradigm
refers to general patterns of thought that tend to shape scientific beliefs during a particular time period
altitude (above horizon)
the angular distance between the horizon and an object in the sky
Arctic Circle
the circle on the Earth with latitude 66.5 degrees N
winter solstice
the point on the celestial sphere where the ecliptic is farthest south of the celestial equator; the moment in time when the Sun appears at that point each year (December 21)
Ptolemaic model
the geocentric model of the universe developed by Ptolemy in about 150 AD
axis tilt
the amount by which a planet's axis is tilted with respect to a line perpendicular to the ecliptic plane
Copernican revolution
the dramatic change that occurred when we learned that Earth is a planet orbiting the Sun rather than the center of the universe
carbon dioxide cycle
the process that cycles carbon dioxide between the Earth's atmosphere and surface rocks
arcminutes
one arcminute is 1/60 of a degree
geocentric model
any of the ancient Greek models that were used to predict planetary positions under the assumption that Earth lay in the center of the universe
paradigm
refers to general patterns of thought that tend to shape scientific beliefs during a particular time period
horizon
a boundary that divides what we can see from what we cannot see
ecliptic
the Sun's apparent annual path among the constellations
eccentricity
a measure of how much an ellipse deviates from a perfect circle; the center-to-focus distance divided by the length of the semimajor axis
spring equinox
the point in Pisces on the celestial sphere where the ecliptic crosses the celestial equator; the moment in time when the Sun appears at that point each year (March 21)
eclipse
occurs when one astronomical object casts a shadow on another or crosses our line of sight to the other object
perihelion
the point at which an object orbiting the Sun is closest to the Sun
angular size (distance)
a measure of the angle formed by extending imaginary lines outward from our eyes to span an object
celestial navigation
navigation on the surface of the Earth accomplished by observations of the Sun and stars
Kepler's first law
states that the orbit of each planet about the Sun is an ellipse with the Sun at one focus
apparent retrograde motion
the apparent motion of a planet, as viewed from Earth, during the period of a few weeks or months when it moves westward relative to the stars in our sky
celestial equator
the extension of the Earth's equator onto the celestial sphere
focus
the point at which rays of light that were initially parallel converge
partial solar eclipse
a solar eclipse during which the Sun becomes only partially blocked by the disk of the Moon
fossil
any relic of an organism that lived and died long ago
celestial coordinates
the coordinates of right ascension and declination that fix an object's position on the celestial sphere
Kepler's laws of planetary motion
three laws discovered by Kepler that describe the motion of the planets around the Sun
retrograde motion
motion that is backward compared to the norm
ellipse
a type of oval that happens to be the shape of bound orbits
nodes
the two points in the Moon's orbit where it crosses the ecliptic plane
solar eclipse
occurs when the Moon's shadow falls on the Earth, which can occur only at new moon
scientific method
an organized approach to explaining observed facts through science
fall equinox
the point in Virgo on the celestial sphere where the ecliptic crosses the celestial equator; the moment in time when the Sun appears at that point each year (September 21)
south celestial pole
the point on the celestial sphere directly above the Earth's South Pole
circumpolar star
a star that always remains above the horizon for a particular latitude
lunar eclipse
occurs when the Moon passes through the Earth's shadow, which can occur only at full moon
theory of evolution
the theory that explains how evolution occurs through the process of natural selection
prime meridian
the meridian of longitude that passes through Greenwich, England, defined to be longitude 0 degrees
local sky
the sky as viewed from a particular location on Earth; objects in the local sky are pinpointed by the coordinates of altitude and azimuth (direction)
stellar parallax
the apparent shift in the position of a nearby star that occurs as we view the star from different positions in the Earth's orbit of the Sun each year
penumbral lunar eclipse
a lunar eclipse in which the Moon passes only within the Earth's penumbral shadow and does not fall within the umbra
apparent solar time
time measured by the actual position of the Sun in your local sky defined so that noon is when the Sun is on the meridian
partial lunar eclipse
a lunar eclipse in which the Moon becomes only partially covered by the Earth's umbral shadow
zenith
the point directly overhead which has an altitude of 90 degrees
saros cycle
the period over which the basic pattern of eclipses repeats (about 18 years and 11 1/3 days)
Kepler's third law
the square of a planet's orbital period is proportional to the cube of its average distance from the Sun (semimajor axis); tells us that more distant planets move more slowly in their orbits
latitude
the angular north-south distance between the Earth's equator and a location on the Earth's surface
Drake Equation
an equation that lays out the factors that play a role in determining the number of communicating civilizations in our galaxy
semimajor axis
half the distance across the long axis of an ellipse (average distance of an orbiting object)
Metonic cycle
the 19 year period over which the lunar phases occur on the same dates
habitable world
a world with environmental conditions under which life could potentially arise or survive
model
a representation of some aspect of nature that can be used to explain and predict real phenomena without invoking myth, magic or the supernatural
geological time scale
the time scale used by scientists to describe major eras in Earth's past
evolution
the gradual change in populations of living organisms responsible for transforming life on Earth from its primitive origins to the great diversity of life today
direction
one of the two coordinates needed to pinpoint an object in the local sky; the direction in which you must face to see the object
geocentric universe
the idea that the Earth is the center of the entire universe
hypothesis
a tentative model proposed to explain some set of observed facts, but which has not yet been rigorously tested and confirmed
total lunar eclipse
a lunar eclipse in which the Moon becomes fully covered by the Earth's umbral shadow
totality
the portion of either a total lunar eclipse during which the Moon is fully within the Earth's umbral shadow or a total solar eclipse during which the Sun's disk is fully blocked by the Moon
habitable zone
the region around a star in which planets could potentially have surface temperatures at which liquid water could exist
celestial sphere
the imaginary sphere on which objects in the sky appear to reside when observed from Earth
umbra
the dark central region of a shadow
Antarctic Circle
the circle on the Earth with latitude 66.5 degrees S
penumbra
the lighter, outlying regions of a shadow
summer solstice
the point on the celestial sphere where the ecliptic is farthest north of the celestial equator; the moment in time when the Sun appears at that point each year (June 21)
zodiac
the constellations on the celestial sphere through which the ecliptic passes