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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. Extends to a distance of 50000AU. Same objects as in the Kuiper belt-when they fall in toward the sun they become comets. Debris from comets hitting the Earths atmosphere cause meteor showers.
Spectroscopic Parallax
Hyashi track
Oort Cloud
partile horizon
2. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
MOONS: thickest atmosphere
E=mc2
Gravitational Lens
Ganymede (Jupiter)
3. Hydrogen and helium (mainly)
Umbra
meteorite
Make up of the jovian planets
Neutron Star
4. A plot of star absolute magnitude verses spectral type.
White Dwarf
Meridian
H-are Diagram
mare basalt
5. The larger bodies that formed early in teh solar nebula that were chemically differentiated
difference between maria and highlands of the moon.
planetesimal
fusion crust
Superior planets
6. 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.
nova
Lagrangian Razor
Autumnal Equinox
Nucleus
7. Extremely round - lots of liquid water - ice rafts on surface ACTIVE SURFACE
coma
Europa (Jupiters moon)
Rich Cluster
MOONS: most geologically active
8. Mercury
contrast northern lowlands and the southern highlands of mars...
Primary Mirror
disk
thinnest atmosphere
9. The lowest energy of an atom.
Ground State
matter dominated universe
Cassini division
Terrestrial Planets
10. A galaxy emitting large amounts of energy at long wavelengths.
radio galaxy
cosmological principle
scarp
tectonics of Earth
11. The location of a supermassive black hole
Nucleus
Self-Propogating Star Formation
CCD
supernova
12. The rock that makes up the lunar highlands
anorthosite
Globular Cluster
Electromagnetic Radiation: Radio
mapping the structure of Milky Way disk
13. The temp at which a substance in the vacuum of space solidifies
Nucleus
superclusters
Umbra
condensation temperature
14. 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?
direct motion
semimajor axis
A family of radiant energy- includes light
15. The family of radiant energy that includes light as a subset
Electromagnetic Radiation
Nucleus
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.
Yes - frozen at the poles- remains protected from the suns rays
16. 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)
Doppler Shift
Cepheid variables
Winter Solstice
contrast northern lowlands and the southern highlands of mars...
17. The relation that tells how light dims with distance.
Inverse Square Law
Jovian Planets
synchronous rotation
Total Eclipse
18. The mix of pure photon energy that emerged at the start of the universe.
300000 KM/sec
cosmic fireball
Cosmic Microwave Background (CMB)
Pulsar
19. A collection of galaxies like the one the Milky Way belongs to
Kuiper belt
CMB
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
Poor Cluster
20. A logarithmically scaled value for the measured brightness of a star.
MOONS: most geologically active
Apparent Magnitude
Reflector
aurora
21. What is the universe expanding into?
gravity
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.
jovian
belt
22. The measure of a variable star's apparent magnitude as it brightens and dims with time
Radio Galaxy
Light Curve
difference between maria and highlands of the moon.
homogeneous
23. 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.
Supercluster
planetary nebula
epicycle
CMB
24. Collections of young - hot stars
OB Associations
mapping the structure of Milky Way disk
zone
Colestial Pole
25. The material from which the solar system formed
most eccentric orbit
quarks
solar nebula
rotation curve = dark matter?
26. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Superior planets
differential rotation
radio galaxy
Sa spiral galaxy
27. A volume of space where few - if any - galaxies are located
Globular Cluster
Void
Astronomical Unit
Seeing
28. A particle of light
Nebula
Pulsar
Big Crunch
Photon
29. Long - meandering cliff formed when a planet surface cools and shrinks
Big Crunch
density
scarp
fastest rotation
30. The process responsible for creating the arms of flocculent spiral galaxies
quasar
H-are Diagram
Self-Propogating Star Formation
Eyepiece Lens
31. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
Titus-Bode Law
tectonics of Earth
highlands
cosmological principle
32. Hydrogen and helium (mainly)
Seeing
Make up of the jovian planets
Parallax
Galilean satellite
33. The equation that describes how matter equates with energy
Gamma-ray Burst
Astronomical Unit
Cosmological Principle
E=mc2
34. 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 variables
CMB
White Dwarf
Negative - Diverge - Less than 1
35. A distance measure determined by the shifting of a star against the background sky every 6 months.
Parsec
Positive - Converge - Greater than 1
Focal Length
Resolving Power
36. The organized effort to find life elsewhere in the universe. (Search for Extra-Terrestrial Intelligence)
A family of radiant energy- includes light
SETI
Supernova (You can be my supernova girl)
interstellar dust
37. Mercury - Venus - Earth - Mars
Terrestrial Planets
Cosmic Microwave Background (CMB)
Primary Mirror
Hipparchus
38. What are the three possible geometries of the universe?
acceleration
Density Wave
Open - flat - and closed.
Self-Propogating Star Formation
39. The area behind a lens where images are resolved
accretion disk
Flocculent spirals
Photosphere
Focal Plane
40. The act of removing an electron from an atom.
Ionization
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.
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.
Oort cloud
41. A crystalline patter found in iron meteorites
Spectroscopic Parallax
widmanstatten pattern
Hydrostatic Equilibrium
Blackbody Curve
42. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Light Gathering Power
Steady State Theory (Leads to Olber's Paradox)
shape and color of SPIRAL galaxies
hottest surface
43. Approximate speed of light in a vacuum
Big Bang
300000 KM/sec
quasar
Light: travels like a wave - detected like a particle
44. Light scattered through the atmosphere that degrades astronomical images
most moons
deferent
Light Pollution
Flat - Flat
45. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
great dark spots
Absolute Magnitude
Ionization
Kuiper belt
46. 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.
regolith
reflection star clusters
We don't know. It might be but does not have to be.
Coronal Loop
47. Electromagnetic Radiation
nucleus
A family of radiant energy- includes light
Cepheid Variable
Ecliptic
48. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
Thermal Equilibrium
blazar
Dark Nebula
bulge
49. The process that powers the sun and hydrogen bombs
Grand design spirals
most moons
Thermonuclear Fusion
Ecliptic
50. 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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