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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. A planet that is closer to the sun than the earth
Supercluster
MOONS: larger than mercury
inferior planets
meteor shower
2. An entity that is likely in the nucleus of most - if not all - galaxies.
hottest surface
Supernova (You can be my supernova girl)
supermassive black hole
MOONS: larger than mercury
3. Electromagnetic Radiation
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.
quasar
great red spot
A family of radiant energy- includes light
4. Sa - Sb galaxies where two magnificent arms wind their way from nucleus out in a symmetrical manner.
Grand design spirals
quasar
Cassegrain Focus
critical density
5. 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.
Big Crunch
Convection
deferent
CMB
6. When the Moon entirely blocks the Sun.
Chromosphere
chondrite
Thermal Equilibrium
Total Eclipse
7. Light-colored high-pressure bands in Jupiter's atmosphere
homogeneous
Cosmic Microwave Background (CMB)
zone
Flat - Flat
8. Dark - reddish - low-pressure bands in Jupiter's atmosphere
Apparent Magnitude
belt
density parameter
Callisto (Jupiter)
9. 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.
Celestial Sphere
Population 1 vs Population 2 stars
greehouse effects
meteoriod
10. Then the Sun moves from north to south across the celestial equator (about September 23)
Autumnal Equinox
Kirchhoff's Law
High Velocity Stars
Asymptotic giant Branch Star
11. The telescope configuration that has the focus placed at the back of the primary mirror
matter dominated universe
synchronous rotation
Electromagnetic Radiation
Cassegrain Focus
12. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
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
Atomic Number
Nova
Negative - Diverge - Less than 1
13. The location of a supermassive black hole
Big Crunch
widmanstatten pattern
Continuous Spectrum
Nucleus
14. The mass of an object divided by its volume
density
Jovian Planets
We don't know. It might be but does not have to be.
Halo
15. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
belt
protostar
tectonics of Venus
Electromagnetic Radiation: X-Ray
16. The high- temperatature outer layer of the sun
Corona
cosmology
Occam's razor
Red Giant Branch Star
17. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
protostar
Parallax
meteor shower
18. Jupiter
MOONS: largest size
fastest rotation
terrestrial planet
opposition
19. The mass of an object divided by its volume
Convection
Coldest surface
aurora
density
20. 1μm 100 nm
Dark matter candidates
Electromagnetic Radiation: Visible Light
Synchrotron Rotation
Trojan asteroids
21. The mix of pure photon energy that emerged at the start of the universe.
meteor
Occam's razor
cosmic fireball
Europa (Jupiters moon)
22. 1 mm 1μm
Gamma ray bursts
Focal Length
Electromagnetic Radiation: Infrared
self-propagating star formation
23. Light scattered through the atmosphere that degrades astronomical images
Chandrasekhar Limit
The Local Group
Light Pollution
Oort Cloud
24. A collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Kuiper belt
Molecular Clouds
Gamma-ray Burst
density parameter
25. The organization of clusters of galaxies into sheets and strings
Supercluster
supermassive black hole
Eclipses of the Moons of Jupiter
Spectroscopic Parallax
26. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
Cosmic Microwave Background
HII Region
Pixel
If it is in a denser medium - such as glass - it will move slower
27. 100 nm 10 nm
Electromagnetic Radiation: Ultraviolet Light
Spectroscopic Parallax
density waves
Continuous Spectrum
28. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
supernova
Dark matter candidates
most moons
Doppler Shift
29. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Main Sequence
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.
Big Bang
Absolute Magnitude
30. The study of the universe as a whole.
Yes - frozen at the poles- remains protected from the suns rays
slowest rotation
cosmology
critical density
31. The gap inthe outer portion of Saturn's A ring
direct motion
Enke gap
Penumbra
blazar
32. A star that blows itself apart
Supernova (You can be my supernova girl)
Photon
Oort cloud
Hyashi track
33. The imaginary sphere centered on the Earth that hols the stars.
Bulge
chemical differentiation
Celestial Sphere
Brown dwarf
34. The name for the only seriously considered theory of the universe.
Quasar
Gravitational Lens
Big Bang
general star population
35. Centered on the Earth
Halo
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Geocentric
tectonics of Mars
36. 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.
Chromosphere
synchrotron radiation
Black Hole
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
37. The mirror that determines the focus configuration of a reflector
Europa (Jupiters moon)
shape and color of SPIRAL galaxies
Self-Propogating Star Formation
Secondary Mirror
38. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Winter Solstice
difference between maria and highlands of the moon.
tectonics of Earth
Light-Year
39. The larger bodies that formed early in teh solar nebula that were chemically differentiated
Largest diameter
E=mc2
planetesimal
SETI
40. What do we think the actual fate of the universe will be and why do we think this?
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.
jovian
interstellar dust
regolith
41. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Halo
shape and color of ELLIPTICAL galaxies
Active Optics
molecular clouds
42. The north-south line passing directly overhead through the zenith.
Meridian
opposition
Kuiper belt
Vernal Equinox
43. A star without enough mass to begin hydrogen fusion
Flat - Remain Parallel - Exactly 1
Corona
Planetary Nebula
Brown dwarf
44. 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.
radio lobe
Sc spiral galaxy
Objective Lens
nova
45. What causes the zones and belts on jupiter and saturn?
mapping the structure of Milky Way disk
Kirkwood gaps
Yes - frozen at the poles- remains protected from the suns rays
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
46. Dark areas on the sun that are cooler than the surrounding photosphere
Sunspots
superclusters
Coldest surface
quasar
47. When material is heated and moves taking the heat energy with it
Secondary Mirror
Magnification
Chromosphere
Convection
48. The force of attraction between any two objects having mass
Ground State
gravity
Parsec
Sb spiral galaxy
49. A faint - remarkably uniform distribution of radiation in space
Main Sequence Stars
Objective Lens
Cosmic Microwave Background
most eccentric orbit
50. Either Io -Europa - Ganymede - or Callisto
AGN
Galilean satellite
Kirchhoff's Law
OB Associations