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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 source of the force that is accelerating the expansion rate of the universe.
general star population
Coldest surface
Grand design spirals
dark energy
2. 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)
Chandrasekhar Limit
MOONS: larger than mercury
How is winding dilemma solved?
mare basalt
3. A term referring to Earth-like planets
terrestrial planet
anorthosite
Photosphere
Supercluster
4. The law that syas light energy from a blackbody increases as (temperature^4)
Stephen-Boltzman Law
rotation curve = dark matter?
Supercluster
planetesimal
5. Any change in the speed or direction of an object's motion
Halo
self-propagating star formation
acceleration
Metals
6. A word meaning 'the same in all directions.'
isotropic
greehouse effects
fusion crust
most eccentric orbit
7. The rock that makes up the lunar highlands
anorthosite
Hyashi track
Radio Galaxy
Doppler Shift
8. Saturn
isotropic
Flocculent spirals
synchronous rotation
least dense
9. The mass of an object divided by its volume
Cosmological Principle
density
HII Region
meteoriod
10. A particle of light
Light Curve
opposition
Photon
Planck time
11. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Seyfert galaxy
Astronomical Unit
nova
mass
12. Elliptical orbits that come inside orbit of the Earth.
Perihelion
Cepheid variables
Apollo asteroids
blazar
13. A star fusing hydrogen to helium in it's core
difference between maria and highlands of the moon.
Main Sequence Stars
Proton-proton chain
The Big Bang Theory resolves Olber's Paradox
14. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
Grand design spirals
Cepheid variables
inferior planets
15. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Colestial Pole
greatest elongation
Blackbody
Titus-Bode Law
16. 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.
deferent
Halo
Seeing
Parallax
17. In Ptolemy's geocentric solar system - the large circle on which a planet's epicycle moved around the Earth.
Poor Cluster
Sc spiral galaxy
deferent
Sunspot cycle
18. The light produced when particles from the sun collide with atmospheric molecules
nova
Photometry
Extrasolar Planet
aurora
19. A term referring to the orbital character of stars near the Sun
Sc spiral galaxy
Differential Rotation
Spectroscopic parallax
Extrasolar Planet
20. A star that blows itself apart
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Supernova (You can be my supernova girl)
density
Spectroscopic parallax
21. The rate of expansion of the universe.
MOONS: largest size
Precession
Hubble constant
cosmic fireball
22. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
mass
Total Eclipse
Sb spiral galaxy
Particle Horizon
23. After stars form they pump light energy into surrounding gas causing it to heat up and glow (H2=ionized hydrogen - H1= neutral hydrogen in molcular couds)
H2 Regions
MOONS: larger than mercury
interstellar dust
plate tectonics
24. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
radiant
Electromagnetic Radiation: Infrared
Sb spiral galaxy
Electromagnetic Radiation: Gamma Ray
25. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Main Sequence
Titus-Bode Law
supermassive black hole
synchrotron radiation
26. What is the universe expanding into?
fastest rotation
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.
Thermonuclear Fusion
rotation curve = dark matter?
27. Population 1 with higher metals and contain many young stars in star clusters. Distribution of stars is everywhere in disk (arms only have 5% more stars)
rotation curve = dark matter?
Magnification
general star population
Population 1 vs Population 2 stars
28. A distance measure determined by the shifting of a star against the background sky every 6 months.
Parsec
Electromagnetic Radiation: Gamma Ray
radio galaxy
neutrino
29. Moon in less than the angular diameter of the Sun.
Annular Eclipse
gravity
Photometry
anorthosite
30. 10^2 nm 10^7 nm
Make up of the jovian planets
Self-Propogating Star Formation
homogeneous
Electromagnetic Radiation: Gamma Ray
31. When a planet lines up with the sun inthe sky
conjunction
Differential Rotation
Primary Mirror
Galilean satellite
32. When particles are compressed to an unnatural state where their pressure is not related to their temperature
rotation curve=winding dilemma?
Degeneracy
Secondary Mirror
Kuiper belt
33. A very dense - highly populated cluster of galaxies
Chromosphere
Oort Cloud
Rich Cluster
Ganymede (Jupiter)
34. A particle of light.
Photon
Eclipses of the Moons of Jupiter
Light: travels like a wave - detected like a particle
Hyashi track
35. When the Moon entirely blocks the Sun.
Total Eclipse
Cepheid variables
accretion
fewest moons
36. 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
Sunspots
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
Kuiper belt
molecular clouds
37. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
retrograde motion
Apollo asteroids
Degeneracy
38. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
density waves
H2 Regions
shape and color of SPIRAL galaxies
differential rotation
39. Rich= dense crowded cores of galaxies - poor= few members and a looser organization of galaxies
Open - flat - and closed.
H2 Regions
Sunspot cycle
Rich vs poor clusters
40. 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)
Observations of distant type Ia supernovae indicate that the expansion of the universe is speeding up with time - not slowing down! So there must be a force causing this.
aphelion
quasar
Open Cluster
41. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
greehouse effects
Big Crunch
Geocentric
Maria
42. The rotation of a star or planet at different speeds at its equator and poles
aphelion
opposition
great dark spots
differential rotation
43. A small spherical dark nebula
Dark matter candidates
Granules
OB Associations
Bok Globule
44. A galaxy emitting large amounts of energy at long wavelengths.
Ground State
Blackbody
Spectroscopic parallax
radio galaxy
45. Any change in the speed or direction of an object's motion
SETI
acceleration
Astronomical Unit
Galilean satellite
46. A younger cluster of stars - found in the galaxy disk
aurora
supernova
Electromagnetic Radiation: Infrared
Open Cluster
47. The crust of a meteorite caused by its entry into Earth's atmosphere
Prominence
Wein's Law
Nucleus
fusion crust
48. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
fusion crust
E=mc2
great red spot
Doppler Shift
49. 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.
superclusters
Convection
CMB
Cosmic Microwave Background
50. Infinitely long -> 10 cm
Electromagnetic Radiation: Radio
greehouse effects
Supercluster
Heliocentric
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