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