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