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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. The movement of the Earth's crustal plates riding on top of the mantle.
Nebula
aphelion
Roundest orbit
plate tectonics
2. A location on an H-are Diagram where evolving stars pulsate
Make up of the terrestrial planets
Electromagnetic Radiation: Microwave
Instability strip
Enke gap
3. 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 _____.
E=mc2
Flat - Remain Parallel - Exactly 1
Electromagnetic Radiation: Gamma Ray
Oort Cloud
4. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Magnification
Cosmic Microwave Background (CMB)
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Halo
5. Originially thought to be stars emitting radio radiation but are now concluded to be nuclei of distant galaxies (same as radio galaxies aka emit streams of material)
Occam's razor
Jupiters red spot
AGN
quasar
6. A younger cluster of stars - found in the galaxy disk
Spectroscopic Parallax
Active Optics
least dense
Open Cluster
7. A perfect absorber and radiator of electromagnetic radiation.
Blackbody
disk
Terrestrial Planets
Degeneracy
8. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
belt
White Dwarf
AGN
Jupiters red spot
9. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
3 reasons we orbit satellites to observe universe
Kirkwood gaps
general star population
radiation dominated universe
10. The apparent path of the Sun through the stars on the celestial sphere.
Magnification
Electromagnetic Radiation: X-Ray
Gamma-ray Burst
Ecliptic
11. The slow wobble of the Earth on its rotation axis.
thinnest atmosphere
Precession
Nova
Liquid metallic hydrogen
12. The rotation period of the Earth measured relative to the Sun.
Summer Solstice
Nebula
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.
Synodic Day
13. A continuous spectrum of light missing energy at a few wave lengths.
Absorption Spectrum
reflection star clusters
Olber's paradox
Flat - Flat
14. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Ground State
Ammonia - methane - and water
Particle Horizon
Blackbody
15. The dark - relativley smooth areas on the moon; Latin for sea
H-are Diagram
solar nebula
Maria
Halo
16. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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17. The crust of a meteorite caused by its entry into Earth's atmosphere
fusion crust
rotation curve = dark matter?
Io (jupiters moon)
Horizontal Branch Star
18. A change in the appearance of the sun at the edge of the solar disk
Coldest surface
Focal Plane
density waves
Limb darkening
19. A telescope that uses mirrors to focus light
cosmic singularity
Focal Plane
inferior planets
Reflector
20. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
Cosmological Principle
Particle Horizon
partile horizon
21. Material that shoots rapidly out into space. Flares cause Auroras
thinnest atmosphere
Flare
If it is in a denser medium - such as glass - it will move slower
Occam's razor
22. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Sb spiral galaxy
cosmology
meteor shower
Photon
23. A rock or iron specimen that has fallen from space
aphelion
homogeneous
Globular Cluster
meteorite
24. Orbit in Jupiters orbit
Chromosphere
Trojan asteroids
Thickest atmosphere
Hydrostatic Equilibrium
25. The faint glow of light left over from the Big Bang. cosmic microwave background are the photons that remain after the big bang that have not turned into matter.
Heliocentric
Light Gathering Power
Heliocentric
CMB
26. A prominence seen against the disk of the sun
Filament
Stephen-Boltzman Law
deferent
Gamma-ray Burst
27. A star that is burning hydrogen to helium in a shell surrounding it's core
Heliocentric
Red Giant Branch Star
Active Optics
terrestrial planet
28. The name for the only seriously considered theory of the universe.
Big Bang
coma
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
force
29. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
Blackbody Curve
Ionization
Coronal Loop
Light: travels like a wave - detected like a particle
30. Infinitely long -> 10 cm
Horizontal Branch Star
Electron
radio galaxy
Electromagnetic Radiation: Radio
31. In what chemical form are jupiters nitrogen - carbon and oxygen?
protostar
AGN
Callisto (Jupiter)
Ammonia - methane - and water
32. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Sb spiral galaxy
cosmic fireball
Heliocentric
synchrotron radiation
33. The elementary building blocks from which protons and neutrons are formed.
quarks
protostar
The Big Bang Theory
Heliocentric
34. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Nova
Geocentric
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Quasar
35. Mercury - Venus - Earth - Mars
Terrestrial Planets
CMB
Sunspot cycle
Spectroscopic Parallax
36. Matter that reveals itself only through its gravitational attraction
Metals
Apparent Magnitude
Dark Matter
High and low pressure which stretch into bands due to the rapid differential rotation. deeper - darker colors are in the belts and zones are lighter
37. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Terrestrial Planets
planetesimal
supermassive black hole
Absorption Spectrum
38. How is the Hubble Law consistent with an expanding universe?
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.
Photon
aurora
Cosmological Principle
39. The relation that tells how light dims with distance.
Jupiters red spot
supermassive black hole
High Velocity Stars
Inverse Square Law
40. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Meridian
quasar
CNO Cycle
High Velocity Stars
41. Large nebula consisting of very cold gas and dust
Steady State Theory (Leads to Olber's Paradox)
CCD
Cassini division
Molecular Clouds
42. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
difference between maria and highlands of the moon.
Open - flat - and closed.
critical density
Ole Roemer
43. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
weight
Absorption Spectrum
300000 KM/sec
mass
44. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
radiation pressure
Self-Propogating Star Formation
Kirchhoff's Law
Photometry
45. When the Sun moves from south to north across the celestial equator (about March 21)
fewest moons
Vernal Equinox
Inverse Square Law
epicycle
46. A galaxy emitting large amounts of energy at long wavelengths.
Blackbody Curve
nova
Emission Spectrum
radio galaxy
47. The equation that describes how matter equates with energy
Objective Lens
fewest moons
accretion
E=mc2
48. The area behind a lens where images are resolved
shape and color of SPIRAL galaxies
Extrasolar Planet
contrast northern lowlands and the southern highlands of mars...
Focal Plane
49. Poitns of gravitational stability in the orbit of a planet
Lagrangian Razor
Electromagnetic Radiation: Radio
nova
Doppler Shift
50. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
Dark matter candidates
neutrino
Liquid metallic hydrogen
direct motion