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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. Centered on the sun.
Heliocentric
Reflector
We don't know. It might be but does not have to be.
Gamma-ray Burst
2. 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
Electromagnetic Radiation: Infrared
contrast northern lowlands and the southern highlands of mars...
supernova
Planetary Nebula
3. Young clusters in disk are irregularly shaped since they have no time to relax into the rounder relaxed shape of globular clusters-will constantly be torn apart and assimilated.
molecular clouds
open star clusters
CMB
Electromagnetic Radiation: Microwave
4. A crystalline patter found in iron meteorites
widmanstatten pattern
Gamma-ray Burst
Hydrostatic Equilibrium
Emission Spectrum
5. A faint - remarkably uniform distribution of radiation in space
Photosphere
Astronomical Unit
Cosmic Microwave Background
gravity
6. Ganymede
radiation dominated universe
cosmological red shift
MOONS: largest size
Globular Cluster
7. A planet that is farther from the sun than the Earth is
Callisto (Jupiter)
Superior planets
self-propagating star formation
Open - flat - and closed.
8. The apparent path of the Sun through the stars on the celestial sphere.
Red Giant Branch Star
Ecliptic
weight
least dense
9. A small and dim but hot star.
disk
Filament
White Dwarf
Electromagnetic Radiation: Radio
10. The rotation period of the Earth measured relative to the Sun.
Synodic Day
Negative - Diverge - Less than 1
SETI
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.
11. Hydrogen and helium (mainly)
Chandrasekhar Limit
Geocentric
Make up of the jovian planets
Thermonuclear Fusion
12. A subatomic particle with a negative charge. It creates light.
aphelion
Supernova (You can be my supernova girl)
Electron
meteor shower
13. The family of radiant energy that includes light as a subset
H-are Diagram
Electromagnetic Radiation
3 reasons we orbit satellites to observe universe
greehouse effects
14. The temp at which a substance in the vacuum of space solidifies
condensation temperature
weight
disk
Colestial Pole
15. Poitns of gravitational stability in the orbit of a planet
Lagrangian Razor
cosmic singularity
opposition
great red spot
16. Titan
most moons
Titus-Bode Law
cosmic singularity
MOONS: thickest atmosphere
17. Electromagnetic Radiation
Main Sequence Stars
Dark matter candidates
A family of radiant energy- includes light
Cosmological Principle
18. The Greek philosopher responsible for making the stellar magnitude scale.
accretion disk
Seyfert galaxy
Objective Lens
Hipparchus
19. A perfect absorber and radiator of electromagnetic radiation.
gravity
Absolute Magnitude
Blackbody
smallest diameter
20. Then the Sun moves from north to south across the celestial equator (about September 23)
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Autumnal Equinox
Vernal Equinox
Density Wave
21. A particle of light
Shepherd satellite
retrograde motion
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Photon
22. Population 1- similar to the sun and 2% of elements are metal - Population 2- formed before gas was metal- only a fraction of mass is metal.
Spectroscopic Parallax
aphelion
Cassegrain Focus
Population 1 vs Population 2 stars
23. The oldest terrain on the moon
Stephen-Boltzman Law
cosmic fireball
highlands
self-propagating star formation
24. Sc galaxies
Drake equation
Flocculent spirals
terrestrial planet
cosmology
25. A star that blows itself apart
Supernova (You can be my supernova girl)
contrast northern lowlands and the southern highlands of mars...
aurora
Big Crunch
26. Half of the longest diameter across an ellipse
Cassini division
If it is in a denser medium - such as glass - it will move slower
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
semimajor axis
27. A measure of the force of gravity on an object
If it is in a denser medium - such as glass - it will move slower
Proton-proton chain
weight
Bulge
28. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Active Optics
superclusters
Light Gathering Power
Stephen-Boltzman Law
29. Plate tectonics due to thickness of crust and maintain their general form when they collide-where most volcanoes are.
Photon
Make up of the terrestrial planets
jovian
tectonics of Earth
30. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
Vernal Equinox
era of recombination
Seyfert galaxy
HII Region
31. Light-flaky crust - convective currents cause it to wrinkle and bunch (1/5 of surface). uniform cratering suggests lack of weathering and tectonics. volcanoes are flat due to atmospheric pressure.
tectonics of Venus
Limb darkening
Bok Globule
Eclipses of the Moons of Jupiter
32. The line on an H-are diagram going from upper left to lower right where normal stars of different masses reside.
Jupiters red spot
Main Sequence
protostar
Winter Solstice
33. An empirical scheme for predictin ghe orbital distances of planets
cosmological red shift
Titus-Bode Law
Annular Eclipse
acceleration
34. The oldest part of the Milky Way
Disk
inferior planets
Heliocentric
Halo
35. The first rock-sized bodies that formed in the solar nebula from dust grains
Energy Level
Hipparchus
Photosphere
chondrite
36. How did Earth come to have an oxygen rich atmosphere?
terrestrial planet
Jupiters red spot
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.
synchronous rotation
37. The part of the Milky way that has on-going star formation
H-are Diagram
Disk
Shepherd satellite
Quasar
38. The law that predicts the possible types of spectra.
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39. A planet orbiting about a distant star
Refractor
Filament
hottest surface
Extrasolar Planet
40. If stars have diff orbital periods - than any arms formed by stars will wind into a tight spiral pattern (billion yrs or so)
Absolute Magnitude
rotation curve=winding dilemma?
Terrestrial Planets
MOONS: thickest atmosphere
41. The process responsible for creating the arms of flocculent spiral galaxies
Self-Propogating Star Formation
MOONS: thickest atmosphere
Atomic Number
Light Gathering Power
42. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
disk
Poor Cluster
Sunspot cycle
great dark spots
43. The location in an H-are diagram of a star cluster - where stars have just left the main sequence. Used to estimate the cluster age.
Autumnal Equinox
Turn off Point
Steady State Theory (Leads to Olber's Paradox)
greehouse effects
44. The measure of a variable star's apparent magnitude as it brightens and dims with time
Radiative Diffusion
Photon
Light Curve
Yes - frozen at the poles- remains protected from the suns rays
45. A plot of star absolute magnitude verses spectral type.
Objective Lens
H-are Diagram
Dark Nebula
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
46. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Jupiters red spot
Io (jupiters moon)
Terrestrial Planets
density parameter
47. A two-filter measure of the color - and hence temperature - of a star.
least dense
Electromagnetic Radiation
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.
Color Index
48. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Electron
Dark Matter
Kuiper belt
acceleration
49. A toroidal or donut-shaped collection of material attracted to a central body like a star or black hole. Dust around an object
The Local Group
Big Bang
accretion disk
The Big Bang Theory resolves Olber's Paradox
50. When massive objects bend space and time enough to create multiple images of an object located behind them
molecular clouds
Gravitational Lens
Instability strip
Poor Cluster