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