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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 very dense - highly populated cluster of galaxies
Dark Matter
era of recombination
Rich Cluster
dark matter
2. The imaginary sphere centered on the Earth that hols the stars.
Nucleus
epicycle
AGN
Celestial Sphere
3. A collection of galaxies like the one the Milky Way belongs to
Occam's razor
Electromagnetic Radiation: Radio
Magnification
Poor Cluster
4. The law that predicts the possible types of spectra.
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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.
Milky way Galaxy
CMB
homogeneous
radio galaxy
6. Large nebula consisting of very cold gas and dust
widmanstatten pattern
High Velocity Stars
Molecular Clouds
Light Curve
7. The light produced when particles from the sun collide with atmospheric molecules
reflection star clusters
Red Giant Branch Star
aurora
direct motion
8. The point directly overhead.
Zenith
Ground State
Flocculent spirals
Precession
9. The apparent path of the Sun through the stars on the celestial sphere.
Sb spiral galaxy
Ecliptic
interstellar dust
Kuiper belt
10. A star that is in the process of forming. It glows from gravitational contraction
Main Sequence Stars
protostar
Photometry
Cosmological Principle
11. The 'edge' of the universe. Light beyond this has not reached us yet.
The Local Group
Oort cloud
contrast northern lowlands and the southern highlands of mars...
partile horizon
12. 10 nm 10^2 nm
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.
Electromagnetic Radiation: X-Ray
Light-Year
coma
13. A faint - remarkably uniform distribution of radiation in space
Sc spiral galaxy
Roundest orbit
Coldest surface
Cosmic Microwave Background
14. A rock or iron specimen that has fallen from space
meteorite
most eccentric orbit
planetesimal
Chandrasekhar Limit
15. A repeated - periodic push or pull capable of summing into a larger push or pull
Cosmic Microwave Background
resonance
tectonics of Mars
smallest diameter
16. 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
aphelion
H-are Diagram
aurora
17. Jupiter
Electromagnetic Radiation: X-Ray
Largest diameter
supermassive black hole
Light Pollution
18. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Sc spiral galaxy
Superior planets
Autumnal Equinox
Disk
19. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Photometry
fusion crust
Thermal Equilibrium
Self-Propogating Star Formation
20. 1μm 100 nm
belt
Electromagnetic Radiation: Visible Light
CMB
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.
21. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Black Hole
Cosmological Principle
Light Gathering Power
Kuiper belt
22. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
radiation dominated universe
Drake equation
most moons
Nova
23. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
open star clusters
Rich vs poor clusters
Doppler Shift
Electromagnetic Radiation: Microwave
24. A small spherical dark nebula
Bok Globule
meteor shower
Radiative Diffusion
Gravitational Lens
25. The source of the force that is accelerating the expansion rate of the universe.
dark energy
Density Wave
Parallax
Make up of the jovian planets
26. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Roundest orbit
interstellar dust
Olber's paradox
radiation pressure
27. The apparent backward motion of a planet against the background of stars.
Plank's Law
bulge
Refractor
retrograde motion
28. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Grand design spirals
Sc spiral galaxy
greatest elongation
Electromagnetic Radiation: Radio
29. Ganymede and Titan
Gravitational Lens
force
Lagrangian Razor
MOONS: larger than mercury
30. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Halo
Eyepiece Lens
Parallax
partile horizon
31. Any change in the speed or direction of an object's motion
slowest rotation
Disk
We don't know. It might be but does not have to be.
acceleration
32. A cool collection of gas and dust silhouetted against a brighter background of stars and/or gas
Dark Nebula
Clouds of sufuric acid (very inhospitable and brightest object in the sky) - process called greenhouse affect traps radiation making it 900 degrees at times - spins with retrograde rotation (sun rises in west) and takes 58.4 days for it to set. Thick
fusion crust
acceleration
33. 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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34. 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.
Plank's Law
partile horizon
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Jupiters red spot
35. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Dark Matter
Spectroscopic Parallax
Objective Lens
Sa spiral galaxy
36. 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)
Proton-proton chain
regolith
molecular clouds
general star population
37. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Ecliptic
Open - flat - and closed.
Sa spiral galaxy
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
38. Heavier elements such as iron - silicon - magnesium - sulfer - nickel
difference between maria and highlands of the moon.
cosmological principle
Dark Matter
Make up of the terrestrial planets
39. When particles are compressed to an unnatural state where their pressure is not related to their temperature
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.
asteroid
Degeneracy
Oort Cloud
40. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
evidence of water on mars
OB Associations
Kuiper belt
difference between maria and highlands of the moon.
41. Mercury
mapping the structure of Milky Way disk
thinnest atmosphere
mass
tectonics of Earth
42. The rock that makes up the lunar maria
density waves
Color Index
blazar
mare basalt
43. The wavelengths where a specific element can absorb or emit light.
Spectral Lines
chondrite
Continuous Spectrum
shape and color of SPIRAL galaxies
44. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Planck time
fastest rotation
Cosmic Microwave Background
Red Giant
45. A planet that is farther from the sun than the Earth is
Doppler Shift
Superior planets
Flocculent spirals
Rich vs poor clusters
46. The Big Bang was not an explosion of matter into empty space - like the explosion of a bomb. Instead - it was an emergence of space and time filled with pure energy where before none of this was present. The point from which is emerged is called the
Lagrangian Razor
The Big Bang Theory
Steady State Theory (Leads to Olber's Paradox)
CMB
47. Dark areas on the sun that are cooler than the surrounding photosphere
Seeing
Hubble law
Most dense
Sunspots
48. The oldest terrain on the moon
solar nebula
molecular clouds
Plague
highlands
49. What is the universe expanding into?
isotropic
Synodic Day
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.
Apollo asteroids
50. The sinking of denser elements to the center of a young molten planet
chemical differentiation
great red spot
Hipparchus
Quasar