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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. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Heliocentric
Sc spiral galaxy
Focal Plane
reflection star clusters
2. What is the universe expanding into?
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.
great dark spots
CNO Cycle
Interstellar Extinction
3. The slow wobble of the Earth on its rotation axis.
solar nebula
Cosmological Principle
Precession
The Big Bang Theory
4. Mercury and venus
hottest surface
Dark matter candidates
general star population
fewest moons
5. A bright area of higher temperature that often proceeds the formation of sunspots.
tectonics of Earth
difference between maria and highlands of the moon.
Plague
Light Curve
6. A plot of star absolute magnitude verses spectral type.
Pixel
H-are Diagram
Stephen-Boltzman Law
Spectroscopy
7. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
3 reasons we orbit satellites to observe universe
Hubble law
opposition
chemical differentiation
8. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
rotation curve = dark matter?
Flocculent spirals
Continuous Spectrum
Halo
9. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
synchrotron radiation
asteroid
accretion
Spectroscopy
10. A planet orbiting about a distant star
Active Optics
Extrasolar Planet
reflection star clusters
Parallax
11. Venus
Main Sequence Stars
Coldest surface
planetesimal
hottest surface
12. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Parsec
zone
Dark Matter
If it is in a denser medium - such as glass - it will move slower
13. Centered on the Earth
superclusters
Ground State
Geocentric
Sb spiral galaxy
14. A term referring to the orbital character of stars near the Sun
deferent
Differential Rotation
Secondary Mirror
Active Optics
15. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Degeneracy
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.
Photometry
Black Hole
16. The powdered stone fragments that make up the lunar 'soil'
regolith
MOONS: thickest atmosphere
Objective Lens
The Big Bang Theory resolves Olber's Paradox
17. What Ole Roemer used to measure the speed of light in a vacuum
Sunspots
Eclipses of the Moons of Jupiter
Kirchhoff's Law
mapping the structure of Milky Way disk
18. A perfect absorber and radiator of electromagnetic radiation.
aphelion
planetesimal
Blackbody
radio galaxy
19. When material is heated and moves taking the heat energy with it
widmanstatten pattern
Asymptotic giant Branch Star
Light Pollution
Convection
20. A huge sphere of tenuous gas surrounding the nucleus of a comet
mapping the structure of Milky Way disk
coma
density parameter
Callisto (Jupiter)
21. The lens that gathers the light in a refractor
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Spectral Lines
Objective Lens
reflection star clusters
22. The apparent path of the Sun through the stars on the celestial sphere.
Pixel
Sunspots
Ecliptic
highlands
23. Collections of young - hot stars
deferent
Nebula
Poor Cluster
OB Associations
24. The light produced when particles from the sun collide with atmospheric molecules
quasar
radio galaxy
Coldest surface
aurora
25. The seasonal shifting of a nearby star's position relative to more distant objects.
Blackbody
mare basalt
conjunction
Parallax
26. The wavelengths where a specific element can absorb or emit light.
Kirkwood gaps
Sunspot cycle
mass
Spectral Lines
27. The area behind a lens where images are resolved
Focal Plane
Thickest atmosphere
quasar
Celestial Equator
28. A star that is in the process of forming. It glows from gravitational contraction
Doppler Shift
planetary nebula
protostar
great dark spots
29. 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 _____.
Flat - Remain Parallel - Exactly 1
Degeneracy
Ole Roemer
Cassegrain Focus
30. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
direct motion
Absolute Magnitude
Supernova (You can be my supernova girl)
3 reasons we orbit satellites to observe universe
31. The science of measuring light energy by wavelength.
The Big Bang Theory resolves Olber's Paradox
Heliocentric
Drake equation
Spectroscopy
32. The dimming of starlight by intervening dust
quasar
Superior planets
reflection star clusters
Interstellar Extinction
33. The rock that makes up the lunar highlands
anorthosite
Bulge
Ecliptic
Electromagnetic Radiation: Microwave
34. When the Sun is farthest north of the celestial equator (about June 22)
Yes - frozen at the poles- remains protected from the suns rays
Summer Solstice
Energy Level
dark matter
35. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
meteoriod
Light Curve
We don't know. It might be but does not have to be.
The Local Group
36. The rotation period of the Earth measured relative to the stars.
Planetary Nebula
Superior planets
matter dominated universe
Sidereal Day
37. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Europa (Jupiters moon)
mare basalt
3 reasons we orbit satellites to observe universe
Nova
38. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
Astronomical Unit
Absorption Spectrum
radiant
39. Mercury
Open - flat - and closed.
smallest diameter
Blackbody Curve
Most dense
40. A star that blows itself apart
Continuous Spectrum
Supernova (You can be my supernova girl)
chemical differentiation
Rich Cluster
41. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
HII Region
Autumnal Equinox
epicycle
Apparent Magnitude
42. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
E=mc2
tectonics of Venus
Turn off Point
tectonics of Earth
43. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
How is winding dilemma solved?
direct motion
Flat - Remain Parallel - Exactly 1
force
44. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Prominence
Eclipses of the Moons of Jupiter
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Electron
45. Light scattered through the atmosphere that degrades astronomical images
Electromagnetic Radiation: Infrared
Light Pollution
Primary Mirror
dark matter
46. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
High Velocity Stars
planetesimal
Population 1 vs Population 2 stars
fewest moons
47. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
The Local Group
Sa spiral galaxy
Apparent Magnitude
Cepheid Variable
48. The movement of the Earth's crustal plates riding on top of the mantle.
Sa spiral galaxy
Convection
weight
plate tectonics
49. When a planet lines up with the sun inthe sky
aurora
conjunction
fastest rotation
Light: travels like a wave - detected like a particle
50. 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
superclusters
interstellar dust
bulge