SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
Test your basic knowledge |
Cosmology
Start Test
Study First
Subject
:
science
Instructions:
Answer 50 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. Collections of young - hot stars
Lagrangian Razor
asteroid
Cassegrain Focus
OB Associations
2. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
MOONS: thickest atmosphere
least dense
density parameter
critical density
3. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
meteorite
Astronomical Unit
Oort cloud
molecular clouds
4. The oldest grouping of stars - found in the galaxy halo
Globular Cluster
Magnification
highlands
Nucleus
5. The point directly overhead.
cosmology
solar nebula
quasar
Zenith
6. The distance between a lens and its focal plane
cosmic fireball
Big Crunch
Focal Length
Extrasolar Planet
7. The shadow behind the Earth or Moon where the Sun is partially obscured.
condensation temperature
Penumbra
synchrotron radiation
radio galaxy
8. The distance light travels in one year (=9.46x10^12km).
H2 Regions
Light-Year
Celestial Sphere
Spectroscopic parallax
9. Mercury
Nebula
smallest diameter
Density Wave
radiant
10. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
isotropic
Parallax
Asymptotic giant Branch Star
Ganymede (Jupiter)
11. A subatomic particle with a negative charge. It creates light.
Poor Cluster
Electron
Wein's Law
Filament
12. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Big Crunch
Neutron Star
greatest elongation
Precession
13. A prominence seen against the disk of the sun
matter dominated universe
tectonics of Mars
greehouse effects
Filament
14. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
3 reasons we orbit satellites to observe universe
Main Sequence
Celestial Sphere
open star clusters
15. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
cosmological red shift
great dark spots
critical density
Coronal Loop
16. The powdered stone fragments that make up the lunar 'soil'
regolith
Blackbody Curve
nova
Halo
17. A term referring to Jupiter-like planets
standard candle
meteorite
jovian
Electromagnetic Radiation: Gamma Ray
18. How did Earth come to have an oxygen rich atmosphere?
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
Supercluster
fastest rotation
open star clusters
19. Jupiter
cosmological principle
Largest diameter
Magnification
Prominence
20. Ganymede and Titan
MOONS: larger than mercury
zone
Grand design spirals
Degeneracy
21. Sc galaxies
Seeing
Flocculent spirals
Neutron Star
Prominence
22. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Cepheid Variable
Oort cloud
rotation curve=winding dilemma?
Planck time
23. How is the Hubble Law consistent with an expanding universe?
direct motion
White Dwarf
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
24. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Radiative Diffusion
Cosmological Principle
neutrino
interstellar dust
25. Radiation given off by electrons accelerating in a magnetic field
Synchrotron Rotation
cosmic fireball
fastest rotation
Dark matter candidates
26. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
Titus-Bode Law
Cosmic Microwave Background (CMB)
Hipparchus
force
27. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Cepheid variables
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
open star clusters
Negative - Diverge - Less than 1
28. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
radio lobe
Thermal Equilibrium
Lagrangian Razor
Flat - Flat
29. Why does the earth have few craters while the moon has many?
Plank's Law
Electromagnetic Radiation: Ultraviolet Light
Yes - frozen at the poles- remains protected from the suns rays
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
30. Matter that reveals itself only through its gravitational attraction.
Thickest atmosphere
HII Region
Metals
dark matter
31. The law that syas light energy from a blackbody increases as (temperature^4)
terrestrial planet
mapping the structure of Milky Way disk
belt
Stephen-Boltzman Law
32. Mercury and venus
terrestrial planet
fewest moons
density parameter
Sa spiral galaxy
33. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
cosmological principle
critical density
blazar
Europa (Jupiters moon)
34. A logarithmically scaled value for the measured brightness of a star.
most eccentric orbit
300000 KM/sec
Apparent Magnitude
Nova
35. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Coronal Loop
Continuous Spectrum
opposition
Largest diameter
36. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
accretion disk
partile horizon
Density Wave
quasar
37. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
It does not have to expand into anything. It might just be that the 3 dimensions of space are getting bigger. It may also be that our 3 spatial dimensions are expanding into higher dimensions if such things exist.
tectonics of Venus
Oort cloud
coma
38. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
great dark spots
Gamma-ray Burst
Corona
39. 10 nm 10^2 nm
Electromagnetic Radiation: X-Ray
Chandrasekhar Limit
Spectroscopic parallax
accretion
40. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
tectonics of Mars
Big Crunch
Limb darkening
Make up of the terrestrial planets
41. Centered on the Earth
Heliocentric
Geocentric
Light Curve
Ammonia - methane - and water
42. The 'edge' of the universe. Light beyond this has not reached us yet.
Light-Year
tectonics of Mars
partile horizon
roche limit
43. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
Hipparchus
SETI
Yes - frozen at the poles- remains protected from the suns rays
Light-Year
44. A star that is burning hydrogen to helium in a shell surrounding it's core
Refractor
Terrestrial Planets
Red Giant Branch Star
Eyepiece Lens
45. The name for the only seriously considered theory of the universe.
Big Bang
Oort cloud
Electromagnetic Radiation: Microwave
radio galaxy
46. The dimming of starlight by intervening dust
molecular clouds
Halo
Planck time
Interstellar Extinction
47. A very dense - highly populated cluster of galaxies
Ammonia - methane - and water
Rich Cluster
We don't know. It might be but does not have to be.
Color Index
48. Moon in less than the angular diameter of the Sun.
critical density
CNO Cycle
Annular Eclipse
superclusters
49. A volume of space where few - if any - galaxies are located
Void
Hyashi track
Ionization
Seyfert galaxy
50. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
asteroid
Molecular Clouds
Flat - Remain Parallel - Exactly 1
Primary Mirror