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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 measure of the ability of a telescope to see fine detail
Resolving Power
Ganymede (Jupiter)
Enke gap
disk
2. A small spherical dark nebula
inferior planets
fusion crust
Bok Globule
OB Associations
3. Venus
hottest surface
Meridian
Open Cluster
roche limit
4. 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)
Dark Matter
Trojan asteroids
Cassini division
Light: travels like a wave - detected like a particle
5. A quantity measuring the stability of the Earth's atmosphere
Ground State
Titus-Bode Law
cosmic fireball
Seeing
6. A small round distribution of gas surrounding a dying star
interstellar dust
Planetary Nebula
Cosmic Microwave Background (CMB)
Cassini division
7. The first rock-sized bodies that formed in the solar nebula from dust grains
Plague
Light-Year
density waves
chondrite
8. The location around an atom where an electron resides.
Coronal Loop
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
Drake equation
Energy Level
9. Poitns of gravitational stability in the orbit of a planet
Lagrangian Razor
shape and color of SPIRAL galaxies
era of recombination
open star clusters
10. What Ole Roemer used to measure the speed of light in a vacuum
Blackbody
Eclipses of the Moons of Jupiter
Electromagnetic Radiation: X-Ray
fusion crust
11. A bridge of material held in position above the solar surface. They can remain for hours even days
The Local Group
Prominence
Make up of the terrestrial planets
Rich Cluster
12. Radiation given off by electrons accelerating in a magnetic field
Rich vs poor clusters
Stephen-Boltzman Law
Synchrotron Rotation
epicycle
13. The distance between a lens and its focal plane
Focal Length
Continuous Spectrum
Wein's Law
Active Optics
14. The law that describes the blackbody curve - and let to quantum mechanics.
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15. Cold aggregates of gas - large and contain a huge amount of matter - so cold that molecules stick together to form molecules.
Meridian
Electromagnetic Radiation: Infrared
molecular clouds
Open - flat - and closed.
16. A galaxy sending out a stream of material from its nucleus
Radio Galaxy
Roundest orbit
neutrino
general star population
17. A planet orbiting about a distant star
epicycle
Flat - Flat
Neutron Star
Extrasolar Planet
18. A measure of the force of gravity on an object
weight
Meridian
cosmological principle
Globular Cluster
19. Titan
mapping the structure of Milky Way disk
aurora
Titus-Bode Law
MOONS: thickest atmosphere
20. The wavelengths where a specific element can absorb or emit light.
self-propagating star formation
matter dominated universe
molecular clouds
Spectral Lines
21. Hot cells of gas that rise and fall in the hotosphere
Quasar
Ammonia - methane - and water
Granules
Negative - Diverge - Less than 1
22. The rate of expansion of the universe.
neutrino
Hubble constant
Drake equation
Halo
23. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
comet
tectonics of Earth
acceleration
tectonics of Earth
24. A large and bright but cool star.
tectonics of Venus
Red Giant
Coronal Loop
weight
25. 10 cm -> 1 mm
Electromagnetic Radiation: Microwave
Gravity only pulls matter back together. Therefore - if gravity is the only force that operates on cosmic scales then the expansion of the universe should decrease with time. The critical density is the value of matter density sufficient to halt the
MOONS: larger than mercury
epicycle
26. Electromagnetic Radiation
A family of radiant energy- includes light
H-are Diagram
Chandrasekhar Limit
nova
27. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Big Crunch
Absolute Magnitude
quasar
protostar
28. The apparent backward motion of a planet against the background of stars.
retrograde motion
Coldest surface
H2 Regions
Kuiper belt
29. A very dense - highly populated cluster of galaxies
differential rotation
Triple Alpha rocess
greatest elongation
Rich Cluster
30. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
nucleus
supernova
Flare
Io (jupiters moon)
31. The apparent path of the Sun through the stars on the celestial sphere.
Thermonuclear Fusion
Zenith
Ecliptic
Autumnal Equinox
32. The powdered stone fragments that make up the lunar 'soil'
MOONS: larger than mercury
Void
Magnification
regolith
33. The dimming of starlight by intervening dust
mass
Interstellar Extinction
coma
Brown dwarf
34. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
Electron
solar nebula
Interstellar Extinction
35. Mercury
most eccentric orbit
Winter Solstice
Horizontal Branch Star
Photon
36. What do we think the actual fate of the universe will be and why do we think this?
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.
Meridian
Chromosphere
radiation pressure
37. Half of the longest diameter across an ellipse
E=mc2
Cassini division
semimajor axis
MOONS: largest size
38. Small moons that maintain the shape of rings around Saturn and Uranus
Shepherd satellite
Limb darkening
Nebula
tectonics of Venus
39. A crystalline patter found in iron meteorites
Red Giant
Winter Solstice
Io (jupiters moon)
widmanstatten pattern
40. Clouds of low density gas often found glowing faintly on either side of an AGN.
radio lobe
coma
Active Optics
condensation temperature
41. The time when the universe cooled sufficiently for atoms to exist. radiation dominated= first 300000 years - THEN era of recombination turns into matter dominated for next.
conjunction
era of recombination
mass
Kuiper belt
42. Moon in less than the angular diameter of the Sun.
Cepheid variables
Ganymede (Jupiter)
Annular Eclipse
Plank's Law
43. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
bulge
shape and color of ELLIPTICAL galaxies
Galilean satellite
Big Crunch
44. The distance light travels in one year (=9.46x10^12km).
Cepheid variables
density
Light-Year
rotation curve=winding dilemma?
45. The 11 or 22 period on the sun durin which sunspots increase - decrease - change polarity - increase and decrease again.
Cosmological Principle
Prominence
Sunspot cycle
slowest rotation
46. The average distance between the Earth and the Sun (=1.5 x10^8km)
highlands
asteroid
Superior planets
Astronomical Unit
47. An entity that is likely in the nucleus of most - if not all - galaxies.
tectonics of Earth
supermassive black hole
Maria
Plague
48. Ganymede
MOONS: largest size
Trojan asteroids
Penumbra
Galilean satellite
49. 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
Globular Cluster
Sc spiral galaxy
The Big Bang Theory
Particle Horizon
50. The temp at which a substance in the vacuum of space solidifies
Zenith
Electromagnetic Radiation: Visible Light
condensation temperature
CMB