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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 process similar to conduction by which energy moves from the solar core to the convective layer
Hubble constant
tectonics of Mars
dark matter
Radiative Diffusion
2. A small and dim but hot star.
aurora
cosmological red shift
White Dwarf
comet
3. 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.
Chromosphere
Apollo asteroids
Turn off Point
Kirchhoff's Law
4. When massive objects bend space and time enough to create multiple images of an object located behind them
greatest elongation
synchronous rotation
least dense
Gravitational Lens
5. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
Flat - Flat
quarks
interstellar dust
evidence of water on mars
6. The number of protons in an atom.
nucleus
Halo
Nebula
Atomic Number
7. A small round distribution of gas surrounding a dying star
H2 Regions
inferior planets
Planetary Nebula
Precession
8. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
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
chondrite
quasar
Positive - Converge - Greater than 1
9. Europa
MOONS: roundest shape
Plague
Particle Horizon
fusion crust
10. A representation of the changes in color and brightness of an evolving protostar.
A family of radiant energy- includes light
comet
Hyashi track
Atomic Number
11. A quantity measuring the stability of the Earth's atmosphere
Triple Alpha rocess
Gamma-ray Burst
Seeing
molecular clouds
12. The Big Bang says that the universe has not existed forever. It had a distinct beginning about 14 billion years ago called the 'Big Bang'. Therefore light from any object more than 14 billion light years away has not had time to reach us. The other p
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183
13. Hot cells of gas that rise and fall in the hotosphere
MOONS: most geologically active
H-are Diagram
HII Region
Granules
14. A younger cluster of stars - found in the galaxy disk
asteroid
Open Cluster
Make up of the jovian planets
CCD
15. Venus
Absolute Magnitude
hottest surface
nucleus
anorthosite
16. The 'edge' of the universe. Light beyond this has not reached us yet.
coma
Electromagnetic Radiation: Gamma Ray
molecular clouds
partile horizon
17. Long - meandering cliff formed when a planet surface cools and shrinks
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
scarp
Flocculent spirals
Thickest atmosphere
18. Very center of galaxy. suggestion of a black hole
Big Bang
Electromagnetic Radiation: Radio
Ecliptic
nucleus
19. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
cosmological red shift
Flat - Flat
Open Cluster
Eyepiece Lens
20. The wavelengths where a specific element can absorb or emit light.
Parallax
Spectral Lines
Extrasolar Planet
cosmic singularity
21. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
direct motion
If it is in a denser medium - such as glass - it will move slower
Light: travels like a wave - detected like a particle
Trojan asteroids
22. As open clusters age - they push gas away but dust remains this can reflect light giving the cluster a blue-ish color. also called reflection nebula
Black Hole
reflection star clusters
Objective Lens
Electromagnetic Radiation: Radio
23. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
How is winding dilemma solved?
opposition
3 reasons we orbit satellites to observe universe
Reflector
24. A very dense - highly populated cluster of galaxies
meteor
Terrestrial Planets
Spectral Lines
Rich Cluster
25. Highlands: rocks are made of lighter anorthosite (similar to old earth rocks) Maria: rocks made of heavy mare basalt (volcanic rock) everywhere else is loose regolith created by meteoric impact.
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
matter dominated universe
difference between maria and highlands of the moon.
300000 KM/sec
26. 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.
H-are Diagram
Coronal Loop
MOONS: roundest shape
Big Bang
27. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
terrestrial planet
Make up of the terrestrial planets
Pixel
Cepheid variables
28. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
Sunspot cycle
tectonics of Earth
shape and color of SPIRAL galaxies
cosmological red shift
29. A galaxy emitting large amounts of energy at long wavelengths.
jovian
aphelion
radio galaxy
Celestial Equator
30. The science of measuring light energy by wavelength.
Spectroscopy
Convection
most moons
Parallax
31. Ganymede
acceleration
MOONS: largest size
partile horizon
Big Crunch
32. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
greatest elongation
plate tectonics
Absolute Magnitude
33. A star that is in the process of forming. It glows from gravitational contraction
protostar
Cosmological Principle
Electron
Dark Matter
34. An important quality of telescopes that increases as the square of the primary mirror or objective lens
greatest elongation
Metals
Light Gathering Power
HII Region
35. A particle of light.
Focal Length
Plague
Photon
accretion disk
36. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Red Giant Branch Star
Population 1 vs Population 2 stars
accretion
most eccentric orbit
37. The crust of a meteorite caused by its entry into Earth's atmosphere
general star population
Ground State
fusion crust
Ole Roemer
38. The location in the Milky Way where stars orbit like a solid wheel
Flat - Flat
MOONS: larger than mercury
Bulge
Magnification
39. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Refractor
Electromagnetic Radiation: Infrared
Limb darkening
Sb spiral galaxy
40. The location of a supermassive black hole
Nucleus
Sc spiral galaxy
300000 KM/sec
Asymptotic giant Branch Star
41. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Degeneracy
Absolute Magnitude
Titus-Bode Law
Negative - Diverge - Less than 1
42. The amount an image is enlarged by a telescope
Galilean satellite
accretion disk
Magnification
supermassive black hole
43. Finding a star's absolute magnitude from it's placement on an HR diagram. After finding the absolute magnitude - we measure the apparent magnitude - for a distance modulus and use this to find the distance. This method is good for finding distances t
Dwarf planets
Light Pollution
homogeneous
Spectroscopic parallax
44. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
Terrestrial Planets
asteroid
blazar
Blackbody
45. The process responsible for creating the arms of flocculent spiral galaxies
Resolving Power
Self-Propogating Star Formation
slowest rotation
direct motion
46. Hydrogen and helium (mainly)
Cepheid Variable
Energy Level
Make up of the jovian planets
Trojan asteroids
47. The area behind a lens where images are resolved
Ganymede (Jupiter)
Prominence
Sidereal Day
Focal Plane
48. 10^2 nm 10^7 nm
Electromagnetic Radiation: Gamma Ray
tectonics of Earth
Instability strip
density waves
49. The telescope configuration that has the focus placed at the back of the primary mirror
tectonics of Mars
E=mc2
Cassegrain Focus
Halo
50. Poitns of gravitational stability in the orbit of a planet
Superior planets
CMB
Molecular Clouds
Lagrangian Razor