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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 Earth
Spectroscopic parallax
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.
Geocentric
retrograde motion
2. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Continuous Spectrum
belt
Sc spiral galaxy
Milky way Galaxy
3. The point in its orbit where a planet is nearest the sun
Perihelion
Gamma-ray Burst
semimajor axis
Most dense
4. A star without enough mass to begin hydrogen fusion
inferior planets
Corona
Brown dwarf
Doppler Shift
5. A logarithmically scaled value for the measured brightness of a star.
The Big Bang Theory resolves Olber's Paradox
terrestrial planet
Cassegrain Focus
Apparent Magnitude
6. The location in the Milky Way where stars orbit like a solid wheel
Nucleus
How is winding dilemma solved?
Neutron Star
Bulge
7. When a planet lines up with the sun inthe sky
conjunction
Red Giant Branch Star
A family of radiant energy- includes light
Ecliptic
8. 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.
Population 1 vs Population 2 stars
CMB
supernova
Jupiters red spot
9. 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
Dwarf planets
reflection star clusters
Plank's Law
mare basalt
10. Why do Galaxies move very rapidly in the interiors of the dense clusters?
MOONS: roundest shape
Continuous Spectrum
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Bulge
11. In a FLAT UNIVERSE(our universe) - the curvature of space-time is ________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
E=mc2
Flat - Remain Parallel - Exactly 1
Nucleus
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
12. A push or a pull
force
conjunction
tectonics of Mars
Gamma ray bursts
13. A two-filter measure of the color - and hence temperature - of a star.
Maria
Color Index
MOONS: roundest shape
density parameter
14. A phenomenon seen when the Earth passes through the orbit of a burned out comet
Horizontal Branch Star
meteor shower
scarp
Red Giant Branch Star
15. The apparent path of the Sun through the stars on the celestial sphere.
Open Cluster
opposition
Ecliptic
MOONS: larger than mercury
16. The shadow behind the Earth or Moon where the Sun is partially obscured.
aphelion
Electromagnetic Radiation: Ultraviolet Light
Penumbra
E=mc2
17. IO
Thermal Equilibrium
Kirkwood gaps
MOONS: most geologically active
Parsec
18. First accurately measured the speed of light in a vacuum
Coronal Loop
planetesimal
direct motion
Ole Roemer
19. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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20. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Focal Length
most eccentric orbit
CCD
quasar
21. Where is the center of the expansion
aurora
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.
Main Sequence Stars
radio galaxy
22. A galaxy sending out a stream of material from its nucleus
radiation dominated universe
hottest surface
quasar
Radio Galaxy
23. A subatomic particle with a negative charge. It creates light.
Electron
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.
Liquid metallic hydrogen
Precession
24. Material that shoots rapidly out into space. Flares cause Auroras
Flare
Focal Plane
matter dominated universe
opposition
25. A particle of light.
Eyepiece Lens
neutrino
weight
Photon
26. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
meteor shower
Instability strip
mass
Photosphere
27. The location in the Milky Way where stars orbit like a solid wheel
difference between maria and highlands of the moon.
Blackbody
Objective Lens
Bulge
28. 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)
general star population
Sa spiral galaxy
Stephen-Boltzman Law
quasar
29. A quantity measuring the stability of the Earth's atmosphere
Seeing
comet
density parameter
contrast northern lowlands and the southern highlands of mars...
30. What are the three possible geometries of the universe?
Open - flat - and closed.
rotation curve = dark matter?
3 reasons we orbit satellites to observe universe
Roundest orbit
31. The act of removing an electron from an atom.
Ionization
Light: travels like a wave - detected like a particle
Thickest atmosphere
SETI
32. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
CNO Cycle
blazar
neutrino
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
33. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
dark energy
Titus-Bode Law
hottest surface
34. 10 nm 10^2 nm
How is winding dilemma solved?
Electromagnetic Radiation: X-Ray
planetesimal
Particle Horizon
35. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Continuous Spectrum
Open Cluster
Callisto (Jupiter)
Brown dwarf
36. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
H-are Diagram
A family of radiant energy- includes light
Colestial Pole
density waves
37. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Milky way Galaxy
Terrestrial Planets
Grand design spirals
Bulge
38. Mercury - Venus - Earth - Mars
Apparent Magnitude
Terrestrial Planets
Cassini division
Largest diameter
39. 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)
Annular Eclipse
general star population
Cepheid Variable
accretion
40. The temp at which a substance in the vacuum of space solidifies
open star clusters
CMB
condensation temperature
quarks
41. The rotation of a star or planet at different speeds at its equator and poles
differential rotation
slowest rotation
Electromagnetic Radiation: X-Ray
Ecliptic
42. Stars fromt he Halo that have drifted into the disk. as earth zooms past them in a faster orbit they appear to be going backward very fast
retrograde motion
High Velocity Stars
Grand design spirals
Oort cloud
43. The elementary building blocks from which protons and neutrons are formed.
quarks
Disk
mass
Milky way Galaxy
44. The point directly overhead.
Ganymede (Jupiter)
Zenith
Cosmological Principle
Galilean satellite
45. The larger bodies that formed early in teh solar nebula that were chemically differentiated
resonance
planetesimal
Spectroscopy
How is winding dilemma solved?
46. Very center of galaxy. suggestion of a black hole
nucleus
Energy Level
asteroid
fewest moons
47. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
We don't know. It might be but does not have to be.
shape and color of SPIRAL galaxies
Occam's razor
Sa spiral galaxy
48. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
Perihelion
Sb spiral galaxy
Primary Mirror
49. A perfect absorber and radiator of electromagnetic radiation.
Blackbody
chemical differentiation
H-are Diagram
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.
50. A measure of the ability of a telescope to see fine detail
Resolving Power
tectonics of Mars
rotation curve = dark matter?
Plague
Sorry!:) No result found.
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