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 speed of light in meters per second. It is also 300 -000 kilometers per second and 186 -000 miles per second.
Orion-Cygnus Arm
300 -000 -000
Galileo Galilei
Binary Star
2. The distance that light travels in one year; about 9.46 trillion kilometers.
Neutron Star
Light Year
Population II Stars
Pulsar
3. The dark lines in a spectrum where light of particular wavelengths has been absorbed.
Cepheid Variable
Neutron Star
Absorption Lines
23:56
4. The older - redder stars that populate a galaxy's hale and bulge. Low metallicity.
Galileo Galilei
Population II Stars
Jovian Planets
Doppler Effect
5. The portion of the Milky Way in which our solar system resides.
Blue Giant
Doppler Effect
Population II Stars
Orion-Cygnus Arm
6. 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
Galactic Bulge
Meteor
Light Year
7. 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.
Redshift
Pulsar
Binary Star
Radiation
8. A rapidly rotating neutron star which emits radiation in magnetic pulses.
Light Year
Meteor
Pulsar
Cepheid Variable
9. Energy that is radiated or transmitted in the form of rays or waves or particles.
Light Year
Nicolaus Copernicus
Radiation
Blue Giant
10. The large - outer planets made of gas - Jupiter - Saturn - Uranus - & Neptune. These all have large moons and rings.
Blue Giant
Red Giant
Terrestrial Planets
Jovian Planets
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.
Calderas
Solstice
Red Giant
Quasar
12. 'Failed' star; a star not massive enough to sustain nuclear fusion.
Brown Dwarf
Neutron Star
Lunar Month
Newton's Laws
13. Polish astronomer who produced a workable heliocentric model of the solar system.
Asterism
Meteor
Nicolaus Copernicus
Parallax
14. Depressions that form when a volcano collapses - as opposed to craters formed by meteoroid impact.
Lunar Month
Nicolaus Copernicus
Solstice
Calderas
15. The small - dense remains of a high-mass star after a supernova.
Neutron Star
Cepheid Variable
Redshift
Nicolaus Copernicus
16. 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.
Newton's Laws
White Dwarf
Galactic Bulge
Galileo Galilei
17. Either of the two times of the year when the Sun is at its greatest distance from the celestial equator.
Nebula
Solstice
23:56
Comet
18. 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
Galactic Bulge
Asterism
Redshift
19. The apparent displacement of an object as seen from two different points that are not on a line with the object.
Absorption Lines
Globular Clusters
Parallax
Ecliptic Plane
20. An orbit that is backward or contrary to the orbital direction of the other planets.
Retrograde
Doppler Effect
Lunar Month
Redshift
21. A relatively small extraterrestrial body consisting of a frozen mass that travels around the Sun in a highly elliptical orbit.
Seyfert Galaxy
Comet
Galactic Bulge
Radiation
22. 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.
Globular Clusters
Radio Galaxy
Solstice
23:56
23. The most precise measurement of Earth's rotation time.
Brown Dwarf
23:56
Blue Giant
Galileo Galilei
24. Italian astronomer and mathematician who was the first to use a telescope to study the stars.
Retrograde
Nicolaus Copernicus
Galileo Galilei
Newton's Laws
25. 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.
Red Giant
Meteor
Comet
Retrograde
26. A cluster of stars (or a small constellation).
Terrestrial Planets
Nebula
Asterism
Pulsar
27. 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.
Orion-Cygnus Arm
Population II Stars
Emission Line
Sunspots
28. The plane of the Earth's orbit around the Sun.
Lunar Month
Parallax
Ecliptic Plane
Cepheid Variable
29. An immense cloud of gas (mainly hydrogen) and dust in interstellar space.
Lunar Month
Nebula
Population II Stars
Emission Line
30. Either of the two celestial points at which the celestial equator intersects the ecliptic plane.
Cepheid Variable
23:56
Ecliptic Plane
Equinox
31. Large - hot - bright star late in the main sequence - having exhausted its hydrogen fuel. Its name comes from its color and size.
Seyfert Galaxy
Blue Giant
Quasar
Galileo Galilei
32. The name given to the four inner planets: Mercury - Venus - Earth - and Mars. Mercury and Venus lack moons.
Terrestrial Planets
White Dwarf
23:56
Meteor
33. A change in the apparent frequency of a wave - as observer and source move toward or away from each other.
23:56
Solstice
Meteor
Doppler Effect
34. A star that expands and cools once it runs out of hydrogen fuel.
Equinox
Terrestrial Planets
Population II Stars
Red Giant
35. Type of active galaxy whose emissions come from a very small region within the nucleus of an otherwise normal-looking spiral system.
Retrograde
Seyfert Galaxy
Equinox
Brown Dwarf
36. 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
Cepheid Variable
Neutron Star
Comet
37. 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
Asterism
Emission Line
23:56
38. 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
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
39. The period between successive new moons (29.531 days).
Blue Giant
300 -000 -000
Lunar Month
Parallax
40. 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.
Electromagnetic Spectrum
White Dwarf
Equinox
Binary Star
41. A narrow - bright region of the spectrum - produced when electrons in atoms jump from one energy level to a lower energy level.
Population I Stars
Doppler Effect
Emission Line
Neutron Star
42. Large - dense groupings of older stars held together by mutual gravitational attraction - which is what keeps them together longer than open clusters.
Globular Clusters
Retrograde
Galactic Bulge
Nebula