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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. Centered on the sun.
Largest diameter
contrast northern lowlands and the southern highlands of mars...
Oort cloud
Heliocentric
2. The law that describes the blackbody curve - and let to quantum mechanics.
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3. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
If it is in a denser medium - such as glass - it will move slower
Seeing
cosmological red shift
Oort Cloud
4. 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.
Celestial Equator
disk
Turn off Point
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
5. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Perihelion
standard candle
Gamma ray bursts
6. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
retrograde motion
condensation temperature
comet
Active Optics
7. The gap inthe outer portion of Saturn's A ring
Proton-proton chain
chemical differentiation
Enke gap
radiation pressure
8. The mirror that determines the focus configuration of a reflector
chemical differentiation
Seeing
Trojan asteroids
Secondary Mirror
9. The oldest grouping of stars - found in the galaxy halo
Make up of the jovian planets
Globular Cluster
Sidereal Day
Oort cloud
10. Long - meandering cliff formed when a planet surface cools and shrinks
cosmology
Continuous Spectrum
Metals
scarp
11. 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)
Rich Cluster
Synchrotron Rotation
H2 Regions
most moons
12. The powdered stone fragments that make up the lunar 'soil'
Objective Lens
Cosmological Principle
regolith
Open - flat - and closed.
13. The sinking of denser elements to the center of a young molten planet
Electromagnetic Radiation: Gamma Ray
High Velocity Stars
chemical differentiation
mass
14. What do we think the actual fate of the universe will be and why do we think this?
quarks
Blackbody
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.
Light-Year
15. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Corona
Stephen-Boltzman Law
Zenith
radio galaxy
16. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Main Sequence
Nebula
critical density
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.
17. The place in the sky that the Earth's axis points toward (can be either north or south)
Filament
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Colestial Pole
Planetary Nebula
18. The part of the Milky way that has on-going star formation
widmanstatten pattern
Gamma-ray Burst
Disk
Focal Length
19. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
synchronous rotation
Electromagnetic Radiation: Ultraviolet Light
Chromosphere
Cosmic Microwave Background (CMB)
20. 10^2 nm 10^7 nm
neutrino
Electromagnetic Radiation: Gamma Ray
Callisto (Jupiter)
cosmological principle
21. The number of protons in an atom.
greatest elongation
contrast northern lowlands and the southern highlands of mars...
highlands
Atomic Number
22. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Main Sequence Stars
Colestial Pole
Flare
greatest elongation
23. Venus (retrograde)
Precession
slowest rotation
Void
Magnification
24. Centered on the Earth
Void
Geocentric
Ammonia - methane - and water
Synchrotron Rotation
25. 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)
Focal Plane
Maria
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
How is winding dilemma solved?
26. Earth
Most dense
Penumbra
CCD
evidence of water on mars
27. The displacement of spectral lines to redder colors caused by the expansion of the universe.
cosmological red shift
asteroid
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.
Colestial Pole
28. That which is responsible for Jupiter's magnetic field
most eccentric orbit
Liquid metallic hydrogen
Thermonuclear Fusion
300000 KM/sec
29. How is the Hubble Law consistent with an expanding universe?
protostar
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
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.
Cosmic Microwave Background
30. A subatomic particle with a negative charge. It creates light.
Color Index
mapping the structure of Milky Way disk
Electron
The Big Bang Theory resolves Olber's Paradox
31. A telescope that uses mirrors to focus light
Reflector
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.
Annular Eclipse
AGN
32. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Cosmic Microwave Background (CMB)
Nova
Largest diameter
Dark Nebula
33. A measure of the force of gravity on an object
fastest rotation
weight
Atomic Number
Maria
34. A star fusing hydrogen to helium in it's core
Brown dwarf
density waves
Main Sequence Stars
Planetary Nebula
35. Jupiter - Saturn - Uranus - Neptune
Jovian Planets
Cosmological Principle
semimajor axis
Chromosphere
36. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Convection
deferent
Sb spiral galaxy
gravity
37. The temp at which a substance in the vacuum of space solidifies
Big Crunch
Hyashi track
condensation temperature
Radiative Diffusion
38. The first rock-sized bodies that formed in the solar nebula from dust grains
Coronal Loop
scarp
chondrite
deferent
39. Jupiter
Ole Roemer
Largest diameter
Thermonuclear Fusion
Cosmic Microwave Background
40. 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.
interstellar dust
Turn off Point
dark matter
Make up of the jovian planets
41. The shadow behind the Earth or Moon where the Sun is partially obscured.
gravity
Penumbra
AGN
gravity
42. 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)
Seyfert galaxy
Interstellar Extinction
general star population
Primary Mirror
43. What are the three possible geometries of the universe?
Electromagnetic Radiation
fusion crust
Open - flat - and closed.
Absolute Magnitude
44. The mirror that determines the focus configuration of a reflector
Secondary Mirror
meteorite
planetesimal
neutrino
45. The location of a supermassive black hole
Sidereal Day
condensation temperature
comet
Nucleus
46. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
highlands
Emission Spectrum
synchrotron radiation
rotation curve = dark matter?
47. Long - meandering cliff formed when a planet surface cools and shrinks
Hubble law
Spectral Lines
scarp
Plank's Law
48. A term referring to the orbital character of stars near the Sun
Largest diameter
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
Dwarf planets
Differential Rotation
49. The fusion process that turns three helium nuclei into a carbon nucleus
terrestrial planet
highlands
Black Hole
Triple Alpha rocess
50. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
neutrino
Secondary Mirror
Thermal Equilibrium