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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 toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
Density Wave
resonance
Steady State Theory (Leads to Olber's Paradox)
accretion disk
2. A long-lived high-pressure bulge in Jupiter's southern hemisphere
Cosmic Microwave Background
Electromagnetic Radiation: Visible Light
great red spot
epicycle
3. A continuous spectrum of light missing energy at a few wave lengths.
A family of radiant energy- includes light
nucleus
Radio Galaxy
Absorption Spectrum
4. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Ganymede (Jupiter)
Interstellar Extinction
dark energy
Pulsar
5. 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.
Limb darkening
aurora
Chandrasekhar Limit
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
6. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Convection
chondrite
Sb spiral galaxy
Light: travels like a wave - detected like a particle
7. A collection of galaxies like the one the Milky Way belongs to
Open - flat - and closed.
Planck time
Poor Cluster
smallest diameter
8. Mercury - Venus - Earth - Mars
MOONS: thickest atmosphere
Hipparchus
Terrestrial Planets
homogeneous
9. 10^2 nm 10^7 nm
highlands
Sb spiral galaxy
Geocentric
Electromagnetic Radiation: Gamma Ray
10. Star speed at outer edge of galaxy should begin to diminish - but they dont so we guess that this means there is increasing force (aka dark matter)
rotation curve = dark matter?
Big Crunch
belt
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.
11. A measure of how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
mass
Thickest atmosphere
Most dense
greehouse effects
12. Either Io -Europa - Ganymede - or Callisto
interstellar dust
Light: travels like a wave - detected like a particle
Galilean satellite
Plank's Law
13. 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
disk
partile horizon
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Magnification
14. Elliptical orbits that come inside orbit of the Earth.
Apollo asteroids
Electromagnetic Radiation: Radio
fastest rotation
Callisto (Jupiter)
15. A planet that is farther from the sun than the Earth is
Doppler Shift
Astronomical Unit
Resolving Power
Superior planets
16. Is space infinitely large?
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17. The family of radiant energy that includes light as a subset
Reflector
isotropic
Bok Globule
Electromagnetic Radiation
18. The apparent path of the Sun through the stars on the celestial sphere.
planetary nebula
MOONS: largest size
Ecliptic
Red Giant
19. The particle horizon is the farthest we can see. It exists because the universe had a beginning and thus a definite age. Light from distances farther away from the particle horizon have not had time to reach us yet.
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Electromagnetic Radiation: Microwave
Particle Horizon
Absolute Magnitude
20. Old - pock marked - icy surface - interior is not differentiated - geologically dead - NOT ACTIVE SURFACE
Magnification
fastest rotation
Callisto (Jupiter)
Cosmic Microwave Background
21. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Autumnal Equinox
Dark matter candidates
Io (jupiters moon)
Apollo asteroids
22. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
Radio Galaxy
Flocculent spirals
Pulsar
Neutron Star
23. The mass of an object divided by its volume
Magnification
Electromagnetic Radiation
density
roche limit
24. The organization of clusters of galaxies into sheets and strings
Cepheid variables
Triple Alpha rocess
Supercluster
Primary Mirror
25. The amount an image is enlarged by a telescope
Granules
Sidereal Day
Magnification
Degeneracy
26. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Galilean satellite
Dark matter candidates
comet
27. The point in its orbit where a planet is nearest the sun
tectonics of Venus
Perihelion
asteroid
Cepheid Variable
28. A perfect absorber and radiator of electromagnetic radiation.
Drake equation
Blackbody
Europa (Jupiters moon)
Make up of the jovian planets
29. Norhern lowlands- darker in color and have far fewer craters as if an ancient sea or ice field covered them. southern highlands- much higher in density of craters.
Trojan asteroids
contrast northern lowlands and the southern highlands of mars...
Photon
highlands
30. The wavelengths where a specific element can absorb or emit light.
Spectral Lines
CCD
meteorite
accretion
31. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
How is winding dilemma solved?
interstellar dust
The Local Group
greehouse effects
32. Arcs of increased mass concentration that slow stars and gas down as they orbit through which cause the formation of stars.
thinnest atmosphere
resonance
density waves
Yes - frozen at the poles- remains protected from the suns rays
33. The distance a moon can be from a planet before shattering from tidal forces
roche limit
solar nebula
Ionization
bulge
34. A very dense - highly populated cluster of galaxies
fewest moons
Summer Solstice
bulge
Rich Cluster
35. The normal eastward movement of a planet against the background of hte distant stars.
Autumnal Equinox
Open Cluster
direct motion
thinnest atmosphere
36. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
planetesimal
fewest moons
Photometry
Instability strip
37. Form honeycomb like patterns surrounding empty or nearly empty voids.
Make up of the jovian planets
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.
superclusters
Synodic Day
38. The material from which the solar system formed
HII Region
solar nebula
Light Curve
Energy Level
39. A bridge of material held in position above the solar surface. They can remain for hours even days
thinnest atmosphere
radio lobe
Lagrangian Razor
Prominence
40. The gap inthe outer portion of Saturn's A ring
Roundest orbit
density
Enke gap
interstellar dust
41. 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
meteoriod
Blackbody Curve
density waves
reflection star clusters
42. A force exerted by reflecting sunlight
Spectroscopy
Grand design spirals
Shepherd satellite
radiation pressure
43. The relation that tells how light dims with distance.
radio galaxy
density waves
Dark Matter
Inverse Square Law
44. 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
Make up of the terrestrial planets
High Velocity Stars
radio galaxy
Olber's paradox
45. Consists of old red stars in slow orbits that plunge through disk and bulge. about 1% are old - round globular clusters.
Ole Roemer
Halo
Focal Plane
Absorption Spectrum
46. Large bulge - tightly wound spiral arms - relatively few h2 regions and are smooth
Open - flat - and closed.
neutrino
MOONS: thickest atmosphere
Sa spiral galaxy
47. 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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48. The high- temperatature outer layer of the sun
Filament
asteroid
Corona
highlands
49. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
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.
dark matter
quasar
Radio Galaxy
50. A subatomic particle with a negative charge. It creates light.
Flocculent spirals
Eyepiece Lens
greatest elongation
Electron