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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. Mercury
most eccentric orbit
Sunspot cycle
radio galaxy
slowest rotation
2. A galaxy sending out a stream of material from its nucleus
Sc spiral galaxy
We don't know. It might be but does not have to be.
Radio Galaxy
Penumbra
3. All possible types of energy that can be emitted and absorbed by atoms.
Big Crunch
mass
Electromagnetic Radiation
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
4. The wavelengths where a specific element can absorb or emit light.
Hipparchus
CMB
Spectral Lines
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
5. A very dense - highly populated cluster of galaxies
300000 KM/sec
The Big Bang Theory
anorthosite
Rich Cluster
6. Earth
Most dense
regolith
Europa (Jupiters moon)
Degeneracy
7. The nuclei of very distant galaxies. Likely a manifestation of supermassive black holes
Gravitational Lens
Stephen-Boltzman Law
Penumbra
Quasar
8. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
meteor shower
Dwarf planets
Cepheid Variable
Light-Year
9. A particle of light
Magnification
Olber's paradox
Neutron Star
Photon
10. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
Superior planets
difference between maria and highlands of the moon.
Light Gathering Power
3 reasons we orbit satellites to observe universe
11. Neptune or uranus
Planck time
radiation dominated universe
H-are Diagram
Coldest surface
12. A collection of galaxies like the one the Milky Way belongs to
Oort Cloud
Poor Cluster
Total Eclipse
Photon
13. 10^2 nm 10^7 nm
Planetary Nebula
accretion disk
Electromagnetic Radiation: Gamma Ray
partile horizon
14. 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.
CMB
Lagrangian Razor
force
Primary Mirror
15. The oldest part of the Milky Way
Halo
Cosmological Principle
AGN
hottest surface
16. The part of the Milky way that has on-going star formation
dark matter
Lagrangian Razor
Disk
epicycle
17. Collections of young - hot stars
SETI
conjunction
Dark matter candidates
OB Associations
18. Europa
MOONS: roundest shape
semimajor axis
cosmic singularity
Pulsar
19. Centered on the Earth
Plank's Law
Milky way Galaxy
Geocentric
synchronous rotation
20. 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
shape and color of SPIRAL galaxies
Heliocentric
chemical differentiation
21. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Dark matter candidates
tectonics of Earth
aurora
Proton-proton chain
22. The gap etween saturn's A and B rings
meteor shower
Cassini division
Emission Spectrum
Main Sequence Stars
23. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Globular Cluster
Callisto (Jupiter)
Electromagnetic Radiation: Visible Light
Red Giant Branch Star
24. A planet orbiting about a distant star
If it is in a denser medium - such as glass - it will move slower
Sa spiral galaxy
Extrasolar Planet
Magnification
25. A star that is burning hydrogen to helium in a shell surrounding it's core
Halo
Electromagnetic Radiation: Ultraviolet Light
Red Giant Branch Star
Hubble law
26. Venus
Roundest orbit
Chromosphere
Color Index
radio galaxy
27. 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?
Light Pollution
critical density
Nova
28. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Nucleus
How is winding dilemma solved?
self-propagating star formation
Seeing
29. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Astronomical Unit
Negative - Diverge - Less than 1
Plague
great dark spots
30. The law that predicts the possible types of spectra.
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183
31. The oldest terrain on the moon
fastest rotation
Ganymede (Jupiter)
highlands
Dark Matter
32. Collections of young - hot stars
Emission Spectrum
roche limit
OB Associations
most moons
33. The rate of expansion of the universe.
shape and color of ELLIPTICAL galaxies
Hubble constant
planetesimal
Thickest atmosphere
34. An evolved star - past the helium flash that is burning helium to carbon in it's cores
Nucleus
Active Optics
Horizontal Branch Star
Radio Galaxy
35. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Red Giant
Open - flat - and closed.
planetary nebula
Planck time
36. Venus
hottest surface
meteor
Open Cluster
quarks
37. Then the Sun moves from north to south across the celestial equator (about September 23)
Ecliptic
radiation dominated universe
Autumnal Equinox
conjunction
38. The science of measuring light energy by wavelength.
Absorption Spectrum
Dark Nebula
Active Optics
Spectroscopy
39. Matter so dense that even light cannot escape its gravity
Grand design spirals
Black Hole
disk
Superior planets
40. The rate of expansion of the universe.
meteor shower
Hubble constant
If it is in a denser medium - such as glass - it will move slower
Continuous Spectrum
41. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Photosphere
Electromagnetic Radiation: Visible Light
evidence of water on mars
Globular Cluster
42. Europa
Red Giant Branch Star
MOONS: roundest shape
Primary Mirror
accretion
43. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Kuiper belt
Flat - Flat
MOONS: largest size
Dark matter candidates
44. The dimming of starlight by intervening dust
Interstellar Extinction
Continuous Spectrum
Autumnal Equinox
Olber's paradox
45. The crust of a meteorite caused by its entry into Earth's atmosphere
general star population
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
OB Associations
fusion crust
46. Small compact stars called white dwarfs can have material deposited on their surfaces. In time material heats up and explodes in surface nuclear reaction- star brightens - settles - repeats.
Eclipses of the Moons of Jupiter
Spectroscopic Parallax
Coldest surface
nova
47. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
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
Nebula
mapping the structure of Milky Way disk
rotation curve = dark matter?
48. Jupiter
Pulsar
anorthosite
quarks
Largest diameter
49. Dark - reddish - low-pressure bands in Jupiter's atmosphere
Roundest orbit
belt
Dark Matter
Cosmological Principle
50. 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.
Cepheid Variable
AGN
CMB
least dense