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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. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
widmanstatten pattern
evidence of water on mars
widmanstatten pattern
dark energy
2. A star fusing hydrogen to helium in it's core
dark energy
least dense
Main Sequence Stars
radiant
3. 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.
Olber's paradox
Absolute Magnitude
cosmological principle
nova
4. The projection of the Earth's equator onto the celestial sphere.
Pulsar
Celestial Equator
Density Wave
cosmic fireball
5. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
opposition
synchrotron radiation
meteor
fewest moons
6. The act of removing an electron from an atom.
Neutron Star
Cassini division
Celestial Equator
Ionization
7. Jupiter - Saturn - Uranus - Neptune
comet
Jovian Planets
Oort cloud
radio galaxy
8. 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
superclusters
conjunction
Light Curve
High Velocity Stars
9. The mirror that determines the focus configuration of a reflector
Secondary Mirror
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
Nova
radio galaxy
10. The first rock-sized bodies that formed in the solar nebula from dust grains
widmanstatten pattern
Ground State
Ammonia - methane - and water
chondrite
11. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Kirkwood gaps
cosmic singularity
nucleus
Olber's paradox
12. Ganymede and Titan
Meridian
MOONS: larger than mercury
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Hubble constant
13. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
opposition
Neutron Star
Hubble law
differential rotation
14. Any class of objects with a uniform luminosity used to determine distance.
epicycle
standard candle
Steady State Theory (Leads to Olber's Paradox)
supernova
15. The shadow behind the Earth or Moon where the Sun is partially obscured.
nova
isotropic
Penumbra
Light Curve
16. Europa
Turn off Point
The Local Group
MOONS: roundest shape
Differential Rotation
17. The sinking of denser elements to the center of a young molten planet
Gravitational Lens
chemical differentiation
Nebula
Refractor
18. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Extrasolar Planet
Halo
The Local Group
terrestrial planet
19. The rotation period of the Earth measured relative to the Sun.
Oort Cloud
Synodic Day
Summer Solstice
Ground State
20. The surface of the sun
synchronous rotation
weight
quarks
Photosphere
21. A huge sphere of tenuous gas surrounding the nucleus of a comet
Halo
Secondary Mirror
coma
Olber's paradox
22. Sc galaxies
Io (jupiters moon)
Flocculent spirals
planetary 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.
23. The north-south line passing directly overhead through the zenith.
Dark Nebula
fusion crust
Meridian
Particle Horizon
24. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Focal Plane
fewest moons
Flare
Parallax
25. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
most moons
evidence of water on mars
Turn off Point
radiation pressure
26. The distance light travels in one year (=9.46x10^12km).
Light-Year
terrestrial planet
Ganymede (Jupiter)
300000 KM/sec
27. The lowest energy of an atom.
Ground State
comet
Kuiper belt
radio lobe
28. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Convection
Maria
Titus-Bode Law
critical density
29. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
planetary nebula
Primary Mirror
Ionization
Thermal Equilibrium
30. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
terrestrial planet
Spectroscopic Parallax
Light Curve
31. The slow wobble of the Earth on its rotation axis.
Rich Cluster
Resolving Power
Precession
Degeneracy
32. 10^2 nm 10^7 nm
Kirchhoff's Law
Electromagnetic Radiation: Gamma Ray
greehouse effects
Objective Lens
33. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Make up of the terrestrial planets
Seyfert galaxy
Cosmic Microwave Background (CMB)
Big Bang
34. The rotation of a star or planet at different speeds at its equator and poles
highlands
greehouse effects
Electromagnetic Radiation
differential rotation
35. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
rotation curve = dark matter?
Atomic Number
Electromagnetic Radiation: Radio
36. The elementary building blocks from which protons and neutrons are formed.
Color Index
quarks
Supercluster
opposition
37. The apparent backward motion of a planet against the background of stars.
Spectroscopic parallax
Rich Cluster
retrograde motion
Ecliptic
38. Dark - reddish - low-pressure bands in Jupiter's atmosphere
meteorite
Ganymede (Jupiter)
belt
highlands
39. The part of the Milky way that has on-going star formation
Eclipses of the Moons of Jupiter
Disk
Refractor
aurora
40. The imaginary sphere centered on the Earth that hols the stars.
aurora
Hyashi track
cosmology
Celestial Sphere
41. Mercury
CNO Cycle
Poor Cluster
smallest diameter
H-are Diagram
42. The linear correlation between the rate of the expansion of the universe and distance. Says that as galaxies get farther away in space - the speed with which they recede from us increases. So we can measure the amount of recessional velocity and use
Thermonuclear Fusion
Hubble law
Main Sequence
Density Wave
43. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Parsec
Positive - Converge - Greater than 1
Light Pollution
Resolving Power
44. 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)
Precession
Void
nucleus
rotation curve = dark matter?
45. The temp at which a substance in the vacuum of space solidifies
condensation temperature
Zenith
Rich vs poor clusters
Energy Level
46. 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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47. Any class of objects with a uniform luminosity used to determine distance.
standard candle
Synodic Day
Light Pollution
dark matter
48. The most mass a white dwarf can have before collapsing to a neutron star
Chandrasekhar Limit
CNO Cycle
force
chemical differentiation
49. An evolved star - past the helium flash that is burning helium to carbon in it's cores
differential rotation
Horizontal Branch Star
Annular Eclipse
weight
50. The imaginary sphere centered on the Earth that hols the stars.
quasar
Celestial Sphere
Self-Propogating Star Formation
rotation curve=winding dilemma?