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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. Is space infinitely large?
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2. Hurricane-like vortex in southern-hemisphere winds to north and south blow in opposite directions which keep it spinning and with no subsurface features like mountians it persists.
Jupiters red spot
Neutron Star
Ground State
Ole Roemer
3. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
molecular clouds
Umbra
White Dwarf
mapping the structure of Milky Way disk
4. The point in its orbit where a planet is farthest from the sun
Sb spiral galaxy
Electromagnetic Radiation
Astronomical Unit
aphelion
5. When the Moon entirely blocks the Sun.
Total Eclipse
Electromagnetic Radiation: Infrared
H-are Diagram
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.
6. A push or a pull
quasar
Light Pollution
force
The Big Bang Theory resolves Olber's Paradox
7. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
H-are Diagram
Sa spiral galaxy
Electromagnetic Radiation: Ultraviolet Light
Asymptotic giant Branch Star
8. Possible Fates of the Universe
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
Perihelion
Meridian
Autumnal Equinox
9. Centered on the Earth
Geocentric
MOONS: most geologically active
Biologicla life created the recycling of nitrogen - co2 - and the production of oxygen. Oxygen is heavier so the atmosphere held onto it easier than hydrogen and helium.
self-propagating star formation
10. Approximate speed of light in a vacuum
thinnest atmosphere
300000 KM/sec
weight
Focal Plane
11. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Secondary Mirror
Ammonia - methane - and water
self-propagating star formation
CCD
12. Light scattered through the atmosphere that degrades astronomical images
Bulge
Ecliptic
Light Pollution
Cepheid Variable
13. Infinitely long -> 10 cm
Milky way Galaxy
Electromagnetic Radiation: Radio
Sunspots
Oort cloud
14. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
The Big Bang Theory resolves Olber's Paradox
Thermal Equilibrium
If it is in a denser medium - such as glass - it will move slower
jovian
15. The layer of the sun just above the photosphere
Big Bang
Umbra
Chromosphere
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
16. Small moons that maintain the shape of rings around Saturn and Uranus
Electromagnetic Radiation
cosmic singularity
Shepherd satellite
accretion
17. The name for the only seriously considered theory of the universe.
highlands
Big Bang
cosmic fireball
Astronomical Unit
18. A long-lived high-pressure bulge in Jupiter's southern hemisphere
great red spot
SETI
Open Cluster
cosmological principle
19. Mercury and venus
Yes - frozen at the poles- remains protected from the suns rays
Nucleus
fewest moons
most eccentric orbit
20. Any change in the speed or direction of an object's motion
acceleration
Negative - Diverge - Less than 1
great dark spots
Objective Lens
21. Sudden blasts of gamma radiation from a very distant galaxy caused possibly by a supernova explosion.
Instability strip
Parsec
Gamma ray bursts
rotation curve = dark matter?
22. That which is responsible for Jupiter's magnetic field
radio galaxy
Grand design spirals
aurora
Liquid metallic hydrogen
23. What causes the zones and belts on jupiter and saturn?
Steady State Theory (Leads to Olber's Paradox)
aphelion
Gamma ray bursts
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
24. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
Superior planets
HII Region
era of recombination
Galilean satellite
25. VENUS
Olber's paradox
retrograde motion
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
Sc spiral galaxy
26. 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 _____.
radiation dominated universe
Flat - Remain Parallel - Exactly 1
meteor shower
Density Wave
27. When the Sun is farthest south of the celestial equator (About December 22)
Sb spiral galaxy
Thermal Equilibrium
Winter Solstice
chemical differentiation
28. The entity from which the whole universe is postulated to have come from.
force
cosmic singularity
critical density
Gravitational Lens
29. What Ole Roemer used to measure the speed of light in a vacuum
Eclipses of the Moons of Jupiter
Thermonuclear Fusion
plate tectonics
Particle Horizon
30. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Radiative Diffusion
Electromagnetic Radiation: X-Ray
Thermonuclear Fusion
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
31. A particle of light
Photon
Ionization
Ammonia - methane - and water
Seeing
32. Moon in less than the angular diameter of the Sun.
Filament
H-are Diagram
thinnest atmosphere
Annular Eclipse
33. The trapping of heat by carbon dioxide or other gases in the Earth's atmosphere.
greehouse effects
blazar
Electromagnetic Radiation: Microwave
Rich vs poor clusters
34. Galaxies whose nuclei emit jets of materil at high speeds. material comes from supermassive black holes
radio galaxy
Sa spiral galaxy
widmanstatten pattern
Cosmic Microwave Background (CMB)
35. 1μm 100 nm
CMB
Electromagnetic Radiation: Visible Light
Electromagnetic Radiation
Big Bang
36. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Doppler Shift
Blackbody Curve
Halo
Liquid metallic hydrogen
37. Sc galaxies
planetesimal
Doppler Shift
Shepherd satellite
Flocculent spirals
38. A rock or iron specimen that has fallen from space
Focal Length
opposition
radio galaxy
meteorite
39. Collections of young - hot stars
Celestial Equator
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.
chondrite
OB Associations
40. The relation that tells how light dims with distance.
Flat - Flat
Inverse Square Law
cosmic singularity
planetary nebula
41. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
3 reasons we orbit satellites to observe universe
Most dense
Blackbody
density parameter
42. The process of acquiring material
accretion
Flat - Remain Parallel - Exactly 1
accretion disk
White Dwarf
43. Centered on the sun.
300000 KM/sec
Synchrotron Rotation
Interstellar Extinction
Heliocentric
44. A galaxy emitting large amounts of energy at long wavelengths.
H-are Diagram
Focal Length
radio galaxy
self-propagating star formation
45. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Globular Cluster
Main Sequence
meteorite
Poor Cluster
46. A star that blows itself apart
Supernova (You can be my supernova girl)
Cepheid Variable
self-propagating star formation
Sidereal Day
47. 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)
cosmic singularity
general star population
accretion disk
most moons
48. The oldest grouping of stars - found in the galaxy halo
blazar
Trojan asteroids
Kirchhoff's Law
Globular Cluster
49. The north-south line passing directly overhead through the zenith.
Meridian
Inverse Square Law
Photon
Ground State
50. An element of a highly efficient - two-dimensional electronic light detector
epicycle
Self-Propogating Star Formation
Pixel
CCD