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Test your basic knowledge |
DSST Astronomy
Start Test
Study First
Subjects
:
dsst
,
science
Instructions:
Answer 42 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. Italian astronomer and mathematician who was the first to use a telescope to study the stars.
Galactic Bulge
Parallax
Galileo Galilei
Neutron Star
2. The portion of the Milky Way in which our solar system resides.
Orion-Cygnus Arm
Galileo Galilei
Ecliptic Plane
Nicolaus Copernicus
3. The plane of the Earth's orbit around the Sun.
Cepheid Variable
Neutron Star
Ecliptic Plane
Sunspots
4. An immense cloud of gas (mainly hydrogen) and dust in interstellar space.
Meteor
Jovian Planets
Nebula
Equinox
5. Large - hot - bright star late in the main sequence - having exhausted its hydrogen fuel. Its name comes from its color and size.
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Ecliptic Plane
Blue Giant
Nicolaus Copernicus
6. The large - outer planets made of gas - Jupiter - Saturn - Uranus - & Neptune. These all have large moons and rings.
Radiation
Jovian Planets
Nicolaus Copernicus
White Dwarf
7. Either of the two times of the year when the Sun is at its greatest distance from the celestial equator.
Meteor
Brown Dwarf
Solstice
Nebula
8. Stage in which a star has used up its helium and its outer layers escape into space - leaving behind a hot - dense core that contracts.
White Dwarf
Emission Line
Population II Stars
Seyfert Galaxy
9. The distance that light travels in one year; about 9.46 trillion kilometers.
Terrestrial Planets
Blue Giant
Light Year
Solstice
10. Depressions that form when a volcano collapses - as opposed to craters formed by meteoroid impact.
Jovian Planets
Pulsar
Calderas
Sunspots
11. Type of active galaxy whose emissions come from a very small region within the nucleus of an otherwise normal-looking spiral system.
Newton's Laws
Seyfert Galaxy
Lunar Month
Meteor
12. Also called nuclear bulge - this is a swelling at the center of spiral galaxies. Bulges consist of old stars and extend out a few thousand light-years from the galactic centers.
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Galactic Bulge
Nicolaus Copernicus
Red Giant
13. The younger stars - some of which are blue - that populate a galaxy's disk - especially its spiral arms. High in heavy metals.
Population II Stars
Redshift
Population I Stars
Quasar
14. A rapidly rotating neutron star which emits radiation in magnetic pulses.
Nicolaus Copernicus
Orion-Cygnus Arm
Population II Stars
Pulsar
15. The apparent displacement of an object as seen from two different points that are not on a line with the object.
Newton's Laws
Emission Line
Galactic Bulge
Parallax
16. A shift in the lines of an object's spectrum toward the red end. It indicates that an object is moving away from the observer. The larger it is - the faster the object is moving.
Globular Clusters
300 -000 -000
Galactic Bulge
Redshift
17. An orbit that is backward or contrary to the orbital direction of the other planets.
Retrograde
Quasar
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Nicolaus Copernicus
18. The speed of light in meters per second. It is also 300 -000 kilometers per second and 186 -000 miles per second.
300 -000 -000
Meteor
Light Year
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19. Short for 'quasi-stellar radio source -' a bright - point-like object that produces the luminosity of 100 to 1 -000 galaxies within a region the size of a solar system.
Ecliptic Plane
Quasar
Doppler Effect
Red Giant
20. Polish astronomer who produced a workable heliocentric model of the solar system.
Retrograde
Ecliptic Plane
Newton's Laws
Nicolaus Copernicus
21. The name given to the four inner planets: Mercury - Venus - Earth - and Mars. Mercury and Venus lack moons.
Emission Line
Galileo Galilei
Terrestrial Planets
Seyfert Galaxy
22. 1. If no forces act on a body - its speed and direction of motion stay constant (an object in motion stays in motion - an object at rest stays at rest). 2. Force=mass x acceleration (F=ma). 3. When two bodies interact - they exert equal and opposite
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23. Areas on the sun's surface that are cooler and less bright than surrounding areas - are caused by the sun's magnetic field - and occur in cycles.
Sunspots
Ecliptic Plane
Red Giant
Radiation
24. Arrangement of electromagnetic radiation--including radio waves - visible light - gamma rays - X-rays - ultraviolet waves - infrared waves - and microwaves--according to their wavelengths.
Electromagnetic Spectrum
Neutron Star
Jovian Planets
Nicolaus Copernicus
25. A narrow - bright region of the spectrum - produced when electrons in atoms jump from one energy level to a lower energy level.
Neutron Star
Meteor
Quasar
Emission Line
26. A star that expands and cools once it runs out of hydrogen fuel.
Solstice
Red Giant
Ecliptic Plane
Cepheid Variable
27. Energy that is radiated or transmitted in the form of rays or waves or particles.
Pulsar
Seyfert Galaxy
Calderas
Radiation
28. A relatively small extraterrestrial body consisting of a frozen mass that travels around the Sun in a highly elliptical orbit.
White Dwarf
Radio Galaxy
Terrestrial Planets
Comet
29. A streak of light in the night sky that results when a meteoroid hits the earth's atmosphere - and air friction causes the meteoroid to melt or vaporize or explode.
Solstice
Comet
Meteor
Equinox
30. The small - dense remains of a high-mass star after a supernova.
Comet
Nebula
Asterism
Neutron Star
31. A cluster of stars (or a small constellation).
Asterism
Orion-Cygnus Arm
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Nicolaus Copernicus
32. The dark lines in a spectrum where light of particular wavelengths has been absorbed.
Solstice
Radiation
Absorption Lines
Sunspots
33. The older - redder stars that populate a galaxy's hale and bulge. Low metallicity.
Cepheid Variable
Equinox
Population II Stars
White Dwarf
34. Large - dense groupings of older stars held together by mutual gravitational attraction - which is what keeps them together longer than open clusters.
Globular Clusters
Sunspots
Terrestrial Planets
Orion-Cygnus Arm
35. A type of pulsating variable star that changes brightness in a regular and predicable manner - making it a useful 'standard candle' for learning absolute magnitudes.
Equinox
Ecliptic Plane
Doppler Effect
Cepheid Variable
36. A pair of stars held together by their mutual gravity and in orbit about each other which can be seen with a telescope as separate objects.
Binary Star
Electromagnetic Spectrum
Equinox
Redshift
37. Either of the two celestial points at which the celestial equator intersects the ecliptic plane.
Lunar Month
Equinox
Population II Stars
Radio Galaxy
38. Very bright - often giant - elliptical galaxy type that emits as much or more energy in the form of radio wavelengths as it does wavelengths of visible light.
Nicolaus Copernicus
Newton's Laws
Radio Galaxy
Electromagnetic Spectrum
39. The period between successive new moons (29.531 days).
Solstice
Quasar
Lunar Month
Meteor
40. 'Failed' star; a star not massive enough to sustain nuclear fusion.
Cepheid Variable
Binary Star
Brown Dwarf
Meteor
41. A change in the apparent frequency of a wave - as observer and source move toward or away from each other.
Blue Giant
Doppler Effect
Brown Dwarf
Lunar Month
42. The most precise measurement of Earth's rotation time.
Meteor
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Terrestrial Planets
Doppler Effect