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