SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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. Mercury
The Big Bang Theory resolves Olber's Paradox
meteor shower
synchrotron radiation
most eccentric orbit
2. The study of the universe as a whole.
cosmology
Apollo asteroids
aurora
great red spot
3. A volume of space where few - if any - galaxies are located
Metals
Void
Limb darkening
Dark Matter
4. Mercury
general star population
Gamma ray bursts
thinnest atmosphere
Maria
5. Dark areas on the sun that are cooler than the surrounding photosphere
Autumnal Equinox
Hydrostatic Equilibrium
Sunspots
Annular Eclipse
6. Radiation given off by electrons accelerating in a magnetic field
Synchrotron Rotation
E=mc2
Resolving Power
Open Cluster
7. 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
Oort Cloud
quasar
Degeneracy
Asymptotic giant Branch Star
8. The rotation period of the Earth measured relative to the stars.
Doppler Shift
highlands
Sidereal Day
Cosmic Microwave Background
9. The material from which the solar system formed
Coldest surface
MOONS: roundest shape
solar nebula
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
10. Theory virtually demands that the geometry of the universe be ______. Results of measuring lumps in the cosmic background radiation indicate that the universe geometry is ________.
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.
differential rotation
Flat - Flat
Spectroscopy
11. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Oort cloud
Umbra
Cassegrain Focus
Big Crunch
12. The mass of an object divided by its volume
Electromagnetic Radiation
Self-Propogating Star Formation
CMB
density
13. 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
Warning
: Invalid argument supplied for foreach() in
/var/www/html/basicversity.com/show_quiz.php
on line
183
14. IO
Hubble law
MOONS: most geologically active
Big Crunch
CCD
15. 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.
Make up of the terrestrial planets
widmanstatten pattern
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.
CMB
16. Clouds of low density gas often found glowing faintly on either side of an AGN.
radio lobe
Hubble constant
Globular Cluster
Light Gathering Power
17. A measure of the ability of a telescope to see fine detail
Dark Nebula
Planck time
Resolving Power
HII Region
18. Jupiter
fastest rotation
anorthosite
E=mc2
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
19. The force of attraction between any two objects having mass
contrast northern lowlands and the southern highlands of mars...
resonance
solar nebula
gravity
20. The point in its orbit where a planet is nearest the sun
cosmological principle
The Local Group
Big Crunch
Perihelion
21. The sinking of denser elements to the center of a young molten planet
Geocentric
Make up of the terrestrial planets
chemical differentiation
planetary nebula
22. The science of measuring light energy by wavelength.
Ground State
opposition
Spectroscopy
mapping the structure of Milky Way disk
23. The era when the ratio of matter to energy greatly favored matter. (verses radiation dominated universe where it was opaque. Matter is now dominated by gravity not photons)
cosmological principle
matter dominated universe
White Dwarf
highlands
24. The gap etween saturn's A and B rings
Autumnal Equinox
Active Optics
Make up of the terrestrial planets
Cassini division
25. A particle of light
Photon
Seyfert galaxy
Kirkwood gaps
retrograde motion
26. Dying large-mass stars lose their outer layers in a violent explosion creating large - chaotic remnants. these brighten like nova but are so much brighter and only occur ONCE PER STAR
Liquid metallic hydrogen
Geocentric
supernova
inferior planets
27. How did Earth come to have an oxygen rich atmosphere?
Sunspots
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.
Inverse Square Law
Stephen-Boltzman Law
28. Infinitely long -> 10 cm
Milky way Galaxy
Electromagnetic Radiation: Radio
Photon
Population 1 vs Population 2 stars
29. 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.
Photon
Jupiters red spot
chondrite
Granules
30. 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)
CCD
general star population
Magnification
Pixel
31. Hot cells of gas that rise and fall in the hotosphere
reflection star clusters
Plank's Law
Granules
density parameter
32. The state of having a balance between inward and outard pressures in a gas--the inward force from gravity is balanced by the outward force from heat.
Hydrostatic Equilibrium
Gamma-ray Burst
plate tectonics
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.
33. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
Vernal Equinox
density waves
Jupiters red spot
critical density
34. The force of attraction between any two objects having mass
cosmic singularity
hottest surface
gravity
self-propagating star formation
35. When the Sun is farthest south of the celestial equator (About December 22)
hottest surface
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Interstellar Extinction
Winter Solstice
36. A plot of star absolute magnitude verses spectral type.
Asymptotic giant Branch Star
H-are Diagram
Bok Globule
Flare
37. In a CLOSED UNIVERSE - the curvature of space-time is _________. Parallel beams will converge/diverge/remain parallel (circle one). The density parameter - Ω0 - is _____.
Superior planets
Focal Length
Positive - Converge - Greater than 1
Horizontal Branch Star
38. The elementary building blocks from which protons and neutrons are formed.
slowest rotation
supernova
quarks
Halo
39. 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)
Main Sequence Stars
mass
Light: travels like a wave - detected like a particle
Interstellar Extinction
40. The law that syas light energy from a blackbody increases as (temperature^4)
direct motion
Black Hole
Inverse Square Law
Stephen-Boltzman Law
41. 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
rotation curve=winding dilemma?
Population 1 vs Population 2 stars
radio lobe
42. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
accretion disk
Thermonuclear Fusion
chemical differentiation
greatest elongation
43. The lens in a telescope used to determine the magnification
Eyepiece Lens
Negative - Diverge - Less than 1
OB Associations
Light Pollution
44. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Photometry
Jupiters red spot
widmanstatten pattern
Electromagnetic Radiation: Radio
45. A streak of light in the atmosphere
meteor
Oort Cloud
terrestrial planet
If it is in a denser medium - such as glass - it will move slower
46. Venus
hottest surface
Autumnal Equinox
Photosphere
Synchrotron Rotation
47. The dark - relativley smooth areas on the moon; Latin for sea
Primary Mirror
least dense
Maria
Photon
48. Half of the longest diameter across an ellipse
Sa spiral galaxy
semimajor axis
homogeneous
retrograde motion
49. A fusion process in which protons build together to form helium
Light Curve
MOONS: most geologically active
Europa (Jupiters moon)
Proton-proton chain
50. A star that is in the process of forming. It glows from gravitational contraction
HII Region
fusion crust
least dense
protostar