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