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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 family of radiant energy that includes light as a subset
Electromagnetic Radiation
Ionization
Chromosphere
H2 Regions
2. 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
force
quarks
H-are Diagram
disk
3. The high- temperatature outer layer of the sun
Corona
Kuiper belt
density
density waves
4. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Asymptotic giant Branch Star
Nova
Electromagnetic Radiation: Visible Light
supernova
5. Dying small mass stars lose their outer layers in a relatively gentle way - creating a round or bipolar nebula about the star (round like planets)
accretion disk
planetary nebula
most moons
quasar
6. Radiation emitted when charged particles spiral rapidly in a magnetic field. come off of jets from black holes.
Liquid metallic hydrogen
synchrotron radiation
radio galaxy
Thermal Equilibrium
7. Massive compact halo objects (MACHO) - weakly interacting massive particles (WIMPY's)
Photosphere
Convection
Dark matter candidates
Liquid metallic hydrogen
8. An entity that is likely in the nucleus of most - if not all - galaxies.
MOONS: larger than mercury
supermassive black hole
zone
Seeing
9. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Differential Rotation
Gamma ray bursts
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
Winter Solstice
10. Dark - reddish - low-pressure bands in Jupiter's atmosphere
Molecular Clouds
belt
Sb spiral galaxy
cosmic singularity
11. A continuous spectrum of light missing energy at a few wave lengths.
Granules
Eclipses of the Moons of Jupiter
Absorption Spectrum
Perihelion
12. A large - irregularly shaped rocky object orbiting the sun mostly between mars and jupiter. Left-over planetesimals
resonance
Cassegrain Focus
asteroid
fastest rotation
13. When particles are compressed to an unnatural state where their pressure is not related to their temperature
Degeneracy
Big Bang
Plank's Law
Atomic Number
14. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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15. A high-pressure bulge in Neptune's southern hemisphere
great dark spots
molecular clouds
Photon
Differential Rotation
16. The final end state of a high mass star. .An entity for which gravity has completely overwhelmed all other forces of nature.
neutrino
terrestrial planet
direct motion
Black Hole
17. Atmosphere blocks high energy wavelengths - atmosphere blurs optical radiation - atmosphere absorbs some radiation at all wavelengths even when it gets through.
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.
mass
3 reasons we orbit satellites to observe universe
comet
18. The fusion process that turns three helium nuclei into a carbon nucleus
Kuiper belt
nucleus
Triple Alpha rocess
shape and color of ELLIPTICAL galaxies
19. The mirror that gathers the light in a reflector
Summer Solstice
Primary Mirror
fusion crust
Penumbra
20. Ganymede
Make up of the terrestrial planets
MOONS: largest size
interstellar dust
3 reasons we orbit satellites to observe universe
21. 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
Apollo asteroids
slowest rotation
The Big Bang Theory
tectonics of Venus
22. Venus (retrograde)
Emission Spectrum
weight
slowest rotation
aurora
23. The mirror that determines the focus configuration of a reflector
Secondary Mirror
Summer Solstice
tectonics of Mars
Supernova (You can be my supernova girl)
24. A collection of galaxies like the one the Milky Way belongs to
Poor Cluster
force
cosmological principle
isotropic
25. A prominence seen against the disk of the sun
semimajor axis
Filament
Superior planets
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
26. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
Sb spiral galaxy
Supercluster
Perihelion
terrestrial planet
27. Matter so dense that even light cannot escape its gravity
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
aurora
Maria
Black Hole
28. Hot cells of gas that rise and fall in the hotosphere
Granules
Cepheid Variable
Ground State
Total Eclipse
29. 10 cm -> 1 mm
Summer Solstice
Electromagnetic Radiation: Microwave
acceleration
Absorption Spectrum
30. 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
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.
slowest rotation
Celestial Equator
31. The mix of pure photon energy that emerged at the start of the universe.
Limb darkening
Thermonuclear Fusion
density
cosmic fireball
32. IO
Flat - Flat
Celestial Equator
MOONS: most geologically active
H2 Regions
33. Wave- only waves cause an interference pattern when passing through a double slit - particle- only particles deposit energy at specific locations (the way an image builds up on digital camera)
tectonics of Earth
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
great red spot
Light: travels like a wave - detected like a particle
34. The distance a moon can be from a planet before shattering from tidal forces
roche limit
MOONS: largest size
Jovian Planets
Poor Cluster
35. A measure of the ability of a telescope to see fine detail
Occam's razor
Molecular Clouds
Blackbody Curve
Resolving Power
36. The distance between a lens and its focal plane
Radio Galaxy
Focal Length
Sunspot cycle
Flare
37. The amount an image is enlarged by a telescope
Parallax
Inverse Square Law
Magnification
Galilean satellite
38. The telescope configuration that has the focus placed at the back of the primary mirror
Rich vs poor clusters
chemical differentiation
Cassegrain Focus
evidence of water on mars
39. The final end state of an intermediate to high mass star. An entity in which all the electrons have been pushed into the protons.
reflection star clusters
chemical differentiation
density parameter
Neutron Star
40. The layer of the sun just above the photosphere
Hubble law
Electromagnetic Radiation: Microwave
general star population
Chromosphere
41. A star without enough mass to begin hydrogen fusion
Negative - Diverge - Less than 1
Brown dwarf
Inverse Square Law
Electromagnetic Radiation: Gamma Ray
42. 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.
Eclipses of the Moons of Jupiter
Particle Horizon
Vernal Equinox
Wein's Law
43. Venus
Thickest atmosphere
Wein's Law
Triple Alpha rocess
evidence of water on mars
44. When the Sun is farthest north of the celestial equator (about June 22)
Pulsar
Kuiper belt
Summer Solstice
Parallax
45. A star that blows itself apart
Spectroscopic Parallax
fewest moons
Supernova (You can be my supernova girl)
Limb darkening
46. The first rock-sized bodies that formed in the solar nebula from dust grains
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
chondrite
chemical differentiation
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
47. A star that is burning hydrogen to helium in a shell surrounding it's core
greatest elongation
Sb spiral galaxy
Light Curve
Red Giant Branch Star
48. 10^2 nm 10^7 nm
Instability strip
bulge
Dark Matter
Electromagnetic Radiation: Gamma Ray
49. Places in the asteroid belt - caused by resonance with Jupiter - where there are no asteroids
Dark Nebula
Neutron Star
Kirkwood gaps
Molecular Clouds
50. A particle of light.
nova
Photon
shape and color of ELLIPTICAL galaxies
Nova