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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. The process responsible for creating the arms of flocculent spiral galaxies
Milky way Galaxy
MOONS: larger than mercury
Self-Propogating Star Formation
quarks
2. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
How is winding dilemma solved?
Refractor
Photometry
general star population
3. A star that is in the process of forming. It glows from gravitational contraction
protostar
Terrestrial Planets
Photosphere
fewest moons
4. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
chemical differentiation
Seeing
Photosphere
5. 10^2 nm 10^7 nm
Shepherd satellite
Synchrotron Rotation
Blackbody Curve
Electromagnetic Radiation: Gamma Ray
6. A fusion process in which protons build together to form helium
Light Pollution
Magnification
least dense
Proton-proton chain
7. Earth
Active Optics
Most dense
Sunspot cycle
Nova
8. The oldest grouping of stars - found in the galaxy halo
Globular Cluster
H-are Diagram
Flat - Remain Parallel - Exactly 1
Gamma ray bursts
9. A logarithmically scaled value for the measured brightness of a star.
reflection star clusters
synchrotron radiation
Apparent Magnitude
Quasar
10. An efficient - two-dimensional electronic light detector. Common in digital cameras - they revolutionized astronomical imaging
CCD
general star population
Neutron Star
Extrasolar Planet
11. In an OPEN UNIVERSE - the curvature of space-time is ____ - Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is____.
Negative - Diverge - Less than 1
Absolute Magnitude
Cepheid variables
Electromagnetic Radiation
12. The crust of a meteorite caused by its entry into Earth's atmosphere
fusion crust
condensation temperature
greatest elongation
Reflector
13. A representation of the changes in color and brightness of an evolving protostar.
direct motion
Hyashi track
Eclipses of the Moons of Jupiter
Black Hole
14. Jupiter
Open - flat - and closed.
Brown dwarf
CCD
most moons
15. 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
supernova
High Velocity Stars
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
inferior planets
16. A younger cluster of stars - found in the galaxy disk
Oort cloud
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
Chromosphere
Open Cluster
17. Saturn
Zenith
Spectroscopic Parallax
least dense
chondrite
18. A small spherical dark nebula
Apollo asteroids
Bok Globule
The Big Bang Theory resolves Olber's Paradox
Shepherd satellite
19. The light produced when particles from the sun collide with atmospheric molecules
Olber's paradox
meteor shower
disk
aurora
20. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
HII Region
AGN
isotropic
roche limit
21. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
Kuiper belt
disk
SETI
Sc spiral galaxy
22. A measure of the ability of a telescope to see fine detail
Ground State
semimajor axis
Resolving Power
era of recombination
23. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
chemical differentiation
aphelion
chemical differentiation
Big Crunch
24. Flat disk with gas - dust - H2 regions - molecular clouds - dust young stars and remnants of old planetary nebula and supernova remnants. stars spin together with similar velocities called differential rotation
Proton-proton chain
disk
meteor shower
inferior planets
25. The lowest energy of an atom.
White Dwarf
Zenith
Absolute Magnitude
Ground State
26. The entity responsible for spiral arms in grand-design spiral galaxies
Vernal Equinox
nova
Instability strip
Density Wave
27. A location on an H-are Diagram where evolving stars pulsate
Electron
Instability strip
Parallax
Black Hole
28. The location of a supermassive black hole
If it is in a denser medium - such as glass - it will move slower
tectonics of Venus
HII Region
Nucleus
29. The apparent path of the Sun through the stars on the celestial sphere.
Quasar
Kirchhoff's Law
Ecliptic
Roundest orbit
30. 10 cm -> 1 mm
Eyepiece Lens
Electromagnetic Radiation: Microwave
Emission Spectrum
Bok Globule
31. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
anorthosite
Parallax
Resolving Power
deferent
32. All wavelengths of light emitted by a blackbody.
Poor Cluster
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.
opposition
Blackbody Curve
33. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
Light-Year
Secondary Mirror
quasar
Continuous Spectrum
34. The first rock-sized bodies that formed in the solar nebula from dust grains
chondrite
Drake equation
Void
H2 Regions
35. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Rich Cluster
accretion disk
Quasar
Parallax
36. The process that powers the sun and hydrogen bombs
Ground State
Ganymede (Jupiter)
Thermonuclear Fusion
cosmological principle
37. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
Titus-Bode Law
comet
MOONS: thickest atmosphere
Flat - Remain Parallel - Exactly 1
38. Ancient stream channels - flood planes - and sedimentary-type rock. Frozen water is found in the polar ice caps and in the soil.
HII Region
Interstellar Extinction
evidence of water on mars
Density Wave
39. The elementary building blocks from which protons and neutrons are formed.
Synodic Day
Nova
Wein's Law
quarks
40. Is space infinitely large?
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41. A perfect absorber and radiator of electromagnetic radiation.
accretion
Blackbody
Gravitational Lens
Black Hole
42. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Hubble constant
radiation dominated universe
coma
quarks
43. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
Plank's Law
Ole Roemer
radio galaxy
Thermonuclear Fusion
44. The assumption that the universe is isotropic (same in all directions) and homogeneous (Same everywhere throughout)
molecular clouds
cosmic singularity
cosmological principle
comet
45. A representation of the changes in color and brightness of an evolving protostar.
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.
accretion disk
Hyashi track
least dense
46. A telescope that uses mirrors to focus light
dark matter
Kirchhoff's Law
Cepheid variables
Reflector
47. 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.
quarks
Sunspot cycle
thinnest atmosphere
Cosmic Microwave Background (CMB)
48. The law that syas light energy from a blackbody increases as (temperature^4)
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
Stephen-Boltzman Law
Flat - Flat
regolith
49. Mercury
most eccentric orbit
Annular Eclipse
Hipparchus
Doppler Shift
50. When the Sun moves from south to north across the celestial equator (about March 21)
Electromagnetic Radiation: Radio
Vernal Equinox
radiation dominated universe
meteoriod