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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 collection of comets in the plane of the solar system - located beyond the orbit of Pluto
Kuiper belt
mapping the structure of Milky Way disk
quarks
Make up of the terrestrial planets
2. The mix of pure photon energy that emerged at the start of the universe.
chemical differentiation
cosmic fireball
Halo
tectonics of Mars
3. Radiation given off by electrons accelerating in a magnetic field
Flare
Synchrotron Rotation
meteoriod
Light Curve
4. Matter so dense that even light cannot escape its gravity
Black Hole
Plague
Drake equation
solar nebula
5. The apparent backward motion of a planet against the background of stars.
Prominence
Precession
retrograde motion
Hydrostatic Equilibrium
6. Centered on the sun.
tectonics of Venus
Heliocentric
interstellar dust
terrestrial planet
7. In what chemical form are jupiters nitrogen - carbon and oxygen?
Ammonia - methane - and water
tectonics of Venus
acceleration
Meridian
8. All wavelengths of light emitted by a blackbody.
Gamma ray bursts
Blackbody Curve
density parameter
Flare
9. The imaginary sphere centered on the Earth that hols the stars.
fusion crust
shape and color of SPIRAL galaxies
Celestial Sphere
Void
10. A change in the wavelength of light caused by a motion between the observer and light (or wave) source (blue shift if getting closer - red shift if moving away)
Doppler Shift
MOONS: roundest shape
dark energy
semimajor axis
11. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
fusion crust
chemical differentiation
tectonics of Venus
epicycle
12. A cloud of ionized hydrogen. Formed when young stars heat the surrounding gas
isotropic
Continuous Spectrum
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
HII Region
13. The mix of pure photon energy that emerged at the start of the universe.
Thermal Equilibrium
Planetary Nebula
cosmic fireball
Wein's Law
14. 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.
CCD
Apparent Magnitude
terrestrial planet
open star clusters
15. The mass of an object divided by its volume
density
Bok Globule
Radio Galaxy
Electromagnetic Radiation: Gamma Ray
16. Flattened spherical distribution of old stars with some young stars too. 'hub' of Milky way - stars orbit with solid body speeds. Elongated into bar shape
weight
Kirchhoff's Law
bulge
Blackbody Curve
17. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
semimajor axis
fusion crust
Ground State
Sc spiral galaxy
18. The ratio of the actual density of the universe to the critical density. (actual density divided by the critical density
Asymptotic giant Branch Star
The Big Bang Theory
density parameter
Open Cluster
19. An evolved star - past the helium flash that is burning helium to carbon in it's cores
neutrino
Horizontal Branch Star
anorthosite
quasar
20. The average distance between the Earth and the Sun (=1.5 x10^8km)
Maria
quasar
Astronomical Unit
aphelion
21. A planet that is farther from the sun than the Earth is
Annular Eclipse
Superior planets
Black Hole
Supercluster
22. Either Io -Europa - Ganymede - or Callisto
Color Index
Electromagnetic Radiation: Infrared
Refractor
Galilean satellite
23. The point directly overhead.
tectonics of Mars
Zenith
Flat - Flat
Active Optics
24. Stars orvits do not define the spiral patterns - instead they are density waves that move at slower speeds (arms are defined by young O and B stars and gas clouds)
Primary Mirror
smallest diameter
fewest moons
How is winding dilemma solved?
25. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
mapping the structure of Milky Way disk
Total Eclipse
rotation curve = dark matter?
26. Is space infinitely large?
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27. Formed rapidly - collapsed slower into disk shape - star birth rate is low but lasts longer and ongoing - contain higher mass blue stars.
most moons
shape and color of SPIRAL galaxies
Electromagnetic Radiation: Gamma Ray
Lagrangian Razor
28. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
Make up of the jovian planets
Io (jupiters moon)
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.
Electron
29. VENUS
inferior planets
synchronous rotation
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
meteor
30. The area behind a lens where images are resolved
blazar
Jovian Planets
Steady State Theory (Leads to Olber's Paradox)
Focal Plane
31. A planet orbiting about a distant star
conjunction
Hydrostatic Equilibrium
Extrasolar Planet
MOONS: largest size
32. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
If it is in a denser medium - such as glass - it will move slower
Big Crunch
White Dwarf
radiant
33. The part of the Milky way that has on-going star formation
Disk
Metals
Parsec
Red Giant Branch Star
34. 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
Globular Cluster
tectonics of Earth
supernova
35. Hydrogen and helium (mainly)
Make up of the jovian planets
Supernova (You can be my supernova girl)
Thickest atmosphere
accretion
36. 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.
Heliocentric
Turn off Point
Halo
accretion disk
37. A term referring to the orbital character of stars near the Sun
fastest rotation
Spectroscopic Parallax
OB Associations
Differential Rotation
38. A continuous spectrum of light missing energy at a few wave lengths.
rotation curve=winding dilemma?
Molecular Clouds
Absorption Spectrum
Globular Cluster
39. Saturn
least dense
Bulge
quasar
Nowhere visible to us. If there are higher dimension then the center would be visible to someone who lives in one. If there are no higher dimensions then the center does not exist.
40. The wavelengths where a specific element can absorb or emit light.
Spectral Lines
synchrotron radiation
Thickest atmosphere
Photometry
41. Venus (retrograde)
Summer Solstice
How is winding dilemma solved?
Ammonia - methane - and water
slowest rotation
42. The imaginary sphere centered on the Earth that hols the stars.
disk
Open - flat - and closed.
Celestial Sphere
Ecliptic
43. The amount an image is enlarged by a telescope
bulge
Geocentric
conjunction
Magnification
44. A star fusing hydrogen to helium in it's core
Main Sequence Stars
Make up of the jovian planets
cosmic singularity
most moons
45. The gap inthe outer portion of Saturn's A ring
Parsec
Neutron Star
Enke gap
Big Crunch
46. The process responsible for creating the arms of flocculent spiral galaxies
Self-Propogating Star Formation
Radiative Diffusion
Light Gathering Power
Photosphere
47. When the Moon entirely blocks the Sun.
least dense
Total Eclipse
nucleus
widmanstatten pattern
48. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Astronomical Unit
interstellar dust
Self-Propogating Star Formation
CMB
49. We can infer the absolute magnitude of pulsating variable stars by measuring their pulsation periods. The longer the pulsations - the greater their luminosities. We then again measure their apparent magnitudes - compare it with their absolute magnitu
Eclipses of the Moons of Jupiter
Cepheid variables
Callisto (Jupiter)
Cassini division
50. The family of radiant energy that includes light as a subset
anorthosite
Globular Cluster
accretion disk
Electromagnetic Radiation