Astronomy Exam I

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Last updated 10:14 PM on 9/20/23
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136 Terms

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What is astronomy

the branch of science that deals with celestial objects in space and the physical universe as a whole

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what is a nebula?

a ball of gas throughout space that gives off color and shapes

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what is a supernova

a star whose life just recently ended, and the aftermath is what’s left of the star/planet

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what is a blackhole?

an enormous amount of mass in a tiny pocket of space that creates a gravity well to where anthing that enters it, won’t come out, including light

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how big is a blackhole?

6 ½ solar masses (or 6.5 times the size of our sun)

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what is the difference between a star and a planet?

a star is a large, glowing ball of gas that generates energy through nuclear fusion in its core, while a planet is a big rock that orbits a star

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on what horizon do stars rise and set?

rise in the east, set in the west

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in the observable universe, how many stars are there?

10 billion trillion stars

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how fast is the speed of light

186,000 miles per second

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a star and all the objects that orbit it

solar system

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the group of galaxies to which the milky way belongs

local group

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the distance light can travel in one year is called a

lightyear

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the largest known structures in the universe, consisting of many clusters of galaxies

supercluster

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the average distance of earth from the sun

astronomical unit

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the orbital motion of one object around another

revolution

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a relatively small, icy object that orbits a star

comet

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a cluster of galaxies

galaxy cluster

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an object that orbits a star but is too small to qualify as a planet or dwarf planet

small solar system body

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the plane of earth’s orbit around the sun

ecliptic plane

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the amount by which a planet’s axis is tilted with respect to a line perpendicular to the ecliptic plane

axis tilt

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the name given to the event thought to mark the birth of the universe

the big bang

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the process which two or smaller nuclei slam together and make one larger nucleus

nuclear fusion

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the portion of the milky way galaxy that is located relatively close to our sun

local solar neighborhood

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the portion of the entire universe that, at least in principle, can be seen from earth

observable universe

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the spinning of an object around its axis

satelite

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the supercluster of galaxies to which the local group belongs

local supercluster

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an object that orbits the sun and is massive enough for gravity to have made it a round shape but does not qualify as a planet because it’s not cleared its orbital neighborhood

a dwarf planet

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alternative name for the universe

cosmos

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local sky

the sky viewed from a particular location on earth

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the portion of a total lunar eclipse during which the moon is fully within Earth’s umbral shadow

totality

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the small circle upon which a planet moves while simultaneously going around a larger circle

epicycle

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a lunar eclipse in which the moon becomes fully covered by earth’s umbral shadow

total lunar eclipse

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a lunar eclipse during which the moon becomes only partially covered by earth’s umbral shadow

partial lunar eclipse

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both the point on the celestial sphere where the ecliptic is farthest south of the celestial equator and the moment in time when the sun appears at that point each year (around december 21)

december solstice

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the sun’s apparent annual path among the constellations

ecliptic

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the gradual wobble of the axis of a rotating object around a vertical line

precession

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a region of the sky

constellations

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a solar eclipse during which the sun becomes only partially blocked by the disk of the moon

partial solar eclipse

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what is the september equinox referred to as?

fall equinox

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direction around the horizon from due north, measured clockwise in degrees

azimuth

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the set of phases in which more and more of the visible face of the moon is becoming illuminated; the phases that come after new moon but before full moon

waxing

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the apparent motion of a planet

apparent retrograde motion

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the set of phases in which less and less of the visible face of the moon is illuminated;

waning

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the dark central region of a shadow

umbra

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a measure of the angle formed by extending imaginary lines outward from our eyes to span an object

angular size

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both the point on the celestial sphere where the ecliptic is farthest north of the celestial equator

june solstice

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the angular distance between the horizon and an object in the sky

altitude

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periods during which lunar and solar eclipses can occur because the nodes of the moon’s orbit are aligned with the earth and the sun

eclipse seasons

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a phase of the moon or a planet

lunar phase

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what is the march equinox referred to as

spring equinox

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an event that occurs when the moon’s shadow falls on earth, which can occur only at new moon

solar eclipse

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1/60 of an arcminute

arcsecond

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the point directly overhead, which has an altitude of 90 degrees

zenith

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both the point in Pisces on the celestial sphere where the ecliptic crosses the celestial equator and the moment in time when the sun appears at that point each year (around march 21)

march equinox

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the constellations on the celestial sphere through which the ecliptic passes

zodiac

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the extension of earth’s equator onto the celestial sphere

celestial equator

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a solar eclipse during which the sun becomes fully blocked by the disk of the moon

total solar eclipse

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the time required for earth to complete exactly one orbit as measured against the stars

sidereal year

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what is the december solstice referred to as?

winter solstice

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an event that occurs when the moon passes through earth’s shadow, which can occur only at full moon

lunar eclipse

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the two points in the moon’s orbit where it crosses the ecliptic plane

nodes

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the apparent shifting of an object against the background, due to viewing it from different positions.

parallax

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the period over which the basic pattern of eclipses repeats, which is about 18 years

saros cycle

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the point on the celestial sphere directly above earth’s south pole

south celestial pole

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a lunar eclipse during which the moon passes only within earth’s penumbral shadow and does not fall within the umbra

penumbral lunar eclipse

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motion that is backward compared to the norm.

retrograde motion

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the lighter, outlying regions of a shadow

penumbra

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the point on the celestial sphere directly above earth’s north pole

north celestial pole

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both the point in virgo on the celestial sphere where the ecliptic crosses the celestial equator and the moment in time when the sun appears at that point each year

september equinox

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24 hours, which is the average time between appearances of the sun on the meridian

solar day

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the circle on earth with latitude 23.5 degrees north, which marks the northernmost latitude at which the sun ever passes directly overhead

tropic of cancer

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1/60 of 1 degree

1 arcminute

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the apparent shift in the position of a nearby star that occurs as we view the star from different poitions in earth’s orbit of the sun each year

stellar parallax

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the phase of the moon in which just a small portion of the visible face is illuminated by sunlight

crescent

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the time of 23 hours 56 mins 4.09 secs between the successive appearance of any particular star on the meridian;

sidereal day

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the meridian of longitude that passes through greenwich england; defined to be longitude 0 degrees

prime meridian

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the angular north-south distance between earth’s equator and a location on earth surface

latitude

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the imaginary sphere on which objects in the sky appear to reside when observed from earth

celestial sphere

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a half-circle extending from your horizon due south, through your zenith, to your horizon due north

meridian

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the rotation of an object that alwats shows the same face to an object that it is orbiting because its rotation period and orbital period are equal

synchronous rotation

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the phase of the moon in which more than half but less than all of the visible face is illuminated by sunlight

gibbous

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a boundary that divides what we can see from what we cannot see

horizon

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the angular east-west distance between the prime meridian and location on earth’s surface

longitude

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a principle used in science, that scientists should prefer two simpler of two models that agree equally well with observations

Occam’s Razor

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the principle that, in the absence of net force, the total momentum of a system remains constant

conservation of momentum

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the acceleration of a falling object

acceleration of gravity

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a general pattern of thought that tends to shape scientific study during a particular time period

paradigm

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the potential energy of mass (E = mc²)

mass-energy

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energy that an object has by virtue of its position in a gravitational field

gravitational potential energy

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the most commonly used temperature scale in science

kelvin

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momentum attribute to rotation or revolution.

angular momentum

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the sum of an orbiting object’s kinetic and gravitational energies

orbital energies

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what is force?

anything that can cause a change in momentum

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the speed necessary for an object to completely escape the gravity of a large body such as a moon, planet or star

escape velocity

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the geocentric model of the universe developed in about 150 A.D.

Ptolemaic Model

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Kepler’s First law

how planets move in elliptical orbits with the sun

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Kepler’s second law

a planet covers the same area of space in the same amount of time no matter where it is in its orbit

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Kepler’s third law

a planet’s orbital period is proportional to the size of it’s orbit

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thermal energy

the collective kinetic energy

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kinetic energy

energy of motion,