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