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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. 'Failed' star; a star not massive enough to sustain nuclear fusion.
Nebula
Brown Dwarf
Retrograde
Equinox
2. The older - redder stars that populate a galaxy's hale and bulge. Low metallicity.
Population II Stars
Nicolaus Copernicus
Newton's Laws
23:56
3. 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.
Electromagnetic Spectrum
Redshift
White Dwarf
Cepheid Variable
4. Italian astronomer and mathematician who was the first to use a telescope to study the stars.
Sunspots
Galileo Galilei
Radiation
Lunar Month
5. The portion of the Milky Way in which our solar system resides.
Orion-Cygnus Arm
Lunar Month
Galactic Bulge
23:56
6. Either of the two times of the year when the Sun is at its greatest distance from the celestial equator.
Terrestrial Planets
300 -000 -000
Emission Line
Solstice
7. Type of active galaxy whose emissions come from a very small region within the nucleus of an otherwise normal-looking spiral system.
Seyfert Galaxy
Blue Giant
Sunspots
Solstice
8. The speed of light in meters per second. It is also 300 -000 kilometers per second and 186 -000 miles per second.
Galactic Bulge
Absorption Lines
Red Giant
300 -000 -000
9. 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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10. A change in the apparent frequency of a wave - as observer and source move toward or away from each other.
Sunspots
Doppler Effect
Parallax
Emission Line
11. Depressions that form when a volcano collapses - as opposed to craters formed by meteoroid impact.
Neutron Star
Globular Clusters
Comet
Calderas
12. 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.
Cepheid Variable
Globular Clusters
Meteor
Population I Stars
13. Either of the two celestial points at which the celestial equator intersects the ecliptic plane.
Radio Galaxy
Terrestrial Planets
Red Giant
Equinox
14. A star that expands and cools once it runs out of hydrogen fuel.
Emission Line
Radiation
Galileo Galilei
Red Giant
15. 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.
Doppler Effect
Seyfert Galaxy
Pulsar
Radio Galaxy
16. 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.
Galactic Bulge
Binary Star
Quasar
Globular Clusters
17. The period between successive new moons (29.531 days).
23:56
Lunar Month
Calderas
Neutron Star
18. The distance that light travels in one year; about 9.46 trillion kilometers.
Light Year
Doppler Effect
Emission Line
Cepheid Variable
19. A relatively small extraterrestrial body consisting of a frozen mass that travels around the Sun in a highly elliptical orbit.
Nicolaus Copernicus
Radiation
Emission Line
Comet
20. The small - dense remains of a high-mass star after a supernova.
Jovian Planets
Neutron Star
Sunspots
Solstice
21. An immense cloud of gas (mainly hydrogen) and dust in interstellar space.
Blue Giant
Galileo Galilei
Seyfert Galaxy
Nebula
22. The plane of the Earth's orbit around the Sun.
Ecliptic Plane
Blue Giant
Terrestrial Planets
Radiation
23. Large - dense groupings of older stars held together by mutual gravitational attraction - which is what keeps them together longer than open clusters.
Globular Clusters
Nicolaus Copernicus
Galileo Galilei
Binary Star
24. Energy that is radiated or transmitted in the form of rays or waves or particles.
Newton's Laws
Population II Stars
Sunspots
Radiation
25. The name given to the four inner planets: Mercury - Venus - Earth - and Mars. Mercury and Venus lack moons.
Newton's Laws
Asterism
Terrestrial Planets
Emission Line
26. A cluster of stars (or a small constellation).
Light Year
Pulsar
Galactic Bulge
Asterism
27. The most precise measurement of Earth's rotation time.
23:56
Parallax
Binary Star
Population II Stars
28. The younger stars - some of which are blue - that populate a galaxy's disk - especially its spiral arms. High in heavy metals.
Population I Stars
23:56
Lunar Month
Binary Star
29. 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.
Quasar
Comet
Red Giant
Emission Line
30. 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.
Doppler Effect
Binary Star
Comet
Sunspots
31. The apparent displacement of an object as seen from two different points that are not on a line with the object.
Parallax
Calderas
Seyfert Galaxy
Radio Galaxy
32. The dark lines in a spectrum where light of particular wavelengths has been absorbed.
Light Year
Absorption Lines
Red Giant
Electromagnetic Spectrum
33. A rapidly rotating neutron star which emits radiation in magnetic pulses.
Pulsar
Equinox
Cepheid Variable
Meteor
34. An orbit that is backward or contrary to the orbital direction of the other planets.
Retrograde
Absorption Lines
Asterism
White Dwarf
35. Large - hot - bright star late in the main sequence - having exhausted its hydrogen fuel. Its name comes from its color and size.
Radiation
Blue Giant
Retrograde
Emission Line
36. A narrow - bright region of the spectrum - produced when electrons in atoms jump from one energy level to a lower energy level.
Equinox
Emission Line
Seyfert Galaxy
Solstice
37. 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
Globular Clusters
Calderas
Ecliptic Plane
38. Arrangement of electromagnetic radiation--including radio waves - visible light - gamma rays - X-rays - ultraviolet waves - infrared waves - and microwaves--according to their wavelengths.
Terrestrial Planets
23:56
Electromagnetic Spectrum
Nebula
39. 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
Population II Stars
Nebula
Solstice
40. Polish astronomer who produced a workable heliocentric model of the solar system.
Nicolaus Copernicus
Binary Star
Ecliptic Plane
Redshift
41. The large - outer planets made of gas - Jupiter - Saturn - Uranus - & Neptune. These all have large moons and rings.
Light Year
Seyfert Galaxy
Jovian Planets
300 -000 -000
42. 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.
Meteor
Red Giant
Parallax
Sunspots