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