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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. 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
Pixel
reflection star clusters
In an expanding universe all galaxies see all other galaxies that are not gravitationally bound to them receding away. This is what we see in the Hubble Law. We infer that the Hubble law also holds true for all other galaxies.
Neutron Star
2. When one side of a body always faces the planet it revolves around
cosmic singularity
synchronous rotation
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
Radio Galaxy
3. The high- temperatature outer layer of the sun
quasar
Perihelion
Corona
nucleus
4. Jupiter
cosmological principle
blazar
Proton-proton chain
Largest diameter
5. The oldest part of the Milky Way
CNO Cycle
molecular clouds
cosmological principle
Halo
6. 1. We see rapid movements or high energy radiation coming at some level from the nuclei of nearly every galaxy we have looked at. 2. We suspect that the creation of these supermassive black holes is part of the galaxy formation process.
Make up of the terrestrial planets
quarks
density
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
7. First accurately measured the speed of light in a vacuum
Steady State Theory (Leads to Olber's Paradox)
Active Optics
Thickest atmosphere
Ole Roemer
8. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Synodic Day
Hipparchus
Io (jupiters moon)
Seeing
9. When material is heated and moves taking the heat energy with it
Active Optics
Convection
Photometry
H-are Diagram
10. The surface of the sun
Photosphere
Plague
era of recombination
mare basalt
11. Is space infinitely large?
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12. The rock that makes up the lunar maria
Shepherd satellite
cosmology
mare basalt
Summer Solstice
13. How did Earth come to have an oxygen rich atmosphere?
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.
Apollo asteroids
meteor shower
matter dominated universe
14. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
Occam's razor
3 reasons we orbit satellites to observe universe
blazar
Objective Lens
15. A very dense - highly populated cluster of galaxies
Rich Cluster
Ecliptic
Dwarf planets
Photometry
16. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
open star clusters
Sunspots
The Local Group
Filament
17. Thick rigid crust - no longer has plate tectonics but still has convective hot spots that create earth-like volcanoes except that last for billions of years because of lack of tectonics.
Perihelion
Make up of the terrestrial planets
rotation curve = dark matter?
tectonics of Mars
18. 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)
quasar
Photosphere
Spectroscopic Parallax
Kuiper belt
19. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Kuiper belt
CNO Cycle
era of recombination
synchronous rotation
20. A location on an H-are Diagram where evolving stars pulsate
Instability strip
MOONS: roundest shape
Corona
Galilean satellite
21. 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.
Turn off Point
Big Crunch
Seyfert galaxy
Terrestrial Planets
22. When massive objects bend space and time enough to create multiple images of an object located behind them
semimajor axis
Gravitational Lens
Shepherd satellite
Seeing
23. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
Zenith
Celestial Equator
Black Hole
24. The rate of expansion of the universe.
Doppler Shift
Hubble constant
Yes - frozen at the poles- remains protected from the suns rays
Galilean satellite
25. Hot cells of gas that rise and fall in the hotosphere
MOONS: thickest atmosphere
3 reasons we orbit satellites to observe universe
Granules
Zenith
26. A small chunk of rock in space
Photon
meteoriod
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.
roche limit
27. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Cassegrain Focus
Light Gathering Power
Sc spiral galaxy
Seyfert galaxy
28. 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
Hipparchus
Instability strip
Self-Propogating Star Formation
Hubble law
29. The law that syas light energy from a blackbody increases as (temperature^4)
Stephen-Boltzman Law
Wein's Law
jovian
Photometry
30. A two-filter measure of the color - and hence temperature - of a star.
Color Index
greatest elongation
Jupiters red spot
hottest surface
31. A planet orbiting about a distant star
great dark spots
Electromagnetic Radiation: Radio
great dark spots
Extrasolar Planet
32. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
matter dominated universe
Population 1 vs Population 2 stars
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.
AGN
33. The surface of the sun
disk
Photosphere
The Big Bang Theory resolves Olber's Paradox
Differential Rotation
34. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Terrestrial Planets
High Velocity Stars
homogeneous
tectonics of Earth
35. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
mass
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.
Secondary Mirror
greatest elongation
36. The amount an image is enlarged by a telescope
jovian
critical density
blazar
Magnification
37. 1 mm 1μm
Electromagnetic Radiation: Infrared
Callisto (Jupiter)
cosmology
CMB
38. A term referring to Jupiter-like planets
Ganymede (Jupiter)
Flat - Remain Parallel - Exactly 1
Objective Lens
jovian
39. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
quasar
Hyashi track
Spectroscopic parallax
Ganymede (Jupiter)
40. When massive objects bend space and time enough to create multiple images of an object located behind them
roche limit
reflection star clusters
Gravitational Lens
Coldest surface
41. Ganymede and Titan
MOONS: larger than mercury
Photon
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.
3 reasons we orbit satellites to observe universe
42. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
A family of radiant energy- includes light
comet
Dwarf planets
Supernova (You can be my supernova girl)
43. The law stating that hotter blackbodies look bluer than cooler blackbodies.
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44. Matter that reveals itself only through its gravitational attraction.
dark matter
force
quasar
Prominence
45. Centered on the sun.
era of recombination
Interstellar Extinction
Electromagnetic Radiation: Ultraviolet Light
Heliocentric
46. The name for the only seriously considered theory of the universe.
Big Bang
Focal Plane
Titus-Bode Law
The Local Group
47. The science of measuring light energy by wavelength.
Cepheid Variable
Ammonia - methane - and water
CNO Cycle
Spectroscopy
48. The number of protons in an atom.
zone
Roundest orbit
MOONS: roundest shape
Atomic Number
49. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
smallest diameter
CCD
Plague
Olber's paradox
50. The point in its orbit where a planet is nearest the sun
Blackbody Curve
Penumbra
Perihelion
era of recombination