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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 apparent backward motion of a planet against the background of stars.
Perihelion
retrograde motion
Photometry
chondrite
2. The science of measuring the apparent magnitudes of stars by imaging them through different filters.
Flat - Flat
Particle Horizon
Photometry
chemical differentiation
3. The imaginary sphere centered on the Earth that hols the stars.
cosmic fireball
Perihelion
Pixel
Celestial Sphere
4. The lens in a telescope used to determine the magnification
Halo
Eyepiece Lens
Electromagnetic Radiation: Infrared
protostar
5. When the Sun is farthest north of the celestial equator (about June 22)
Open Cluster
Absorption Spectrum
Summer Solstice
Gravitational Lens
6. A technique using computer-controlled mirrors to sharpen images distorted by the atmosphere
Active Optics
Primary Mirror
Big Crunch
open star clusters
7. The lowest energy of an atom.
great red spot
Sunspots
Photosphere
Ground State
8. The apparent path of the Sun through the stars on the celestial sphere.
Ecliptic
Dark Matter
Spectral Lines
Electromagnetic Radiation: Gamma Ray
9. Possible Fates of the Universe
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
radio galaxy
nova
isotropic
10. When a planet lines up with the sun inthe sky
conjunction
tectonics of Venus
Steady State Theory (Leads to Olber's Paradox)
Summer Solstice
11. Sc galaxies where star formation and destruction is so rapid that supernova explosions are mainly responsible for compressing gas to create new stars.
Europa (Jupiters moon)
self-propagating star formation
asteroid
Radio Galaxy
12. Hot cells of gas that rise and fall in the hotosphere
Yes - frozen at the poles- remains protected from the suns rays
Granules
dark energy
Open Cluster
13. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
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
neutrino
meteoriod
Io (jupiters moon)
14. A star fusing hydrogen to helium in it's core
planetary nebula
Molecular Clouds
Main Sequence Stars
quasar
15. The seasonal shifting of a nearby star's position relative to more distant objects.
Neutron Star
Parallax
dark energy
weight
16. Poitns of gravitational stability in the orbit of a planet
AGN
Celestial Sphere
Nova
Lagrangian Razor
17. Mercury - Venus - Earth - Mars
radio galaxy
Terrestrial Planets
supermassive black hole
Radio Galaxy
18. Very center of galaxy. suggestion of a black hole
nucleus
Blackbody Curve
Coldest surface
Granules
19. A planet that is closer to the sun than the earth
Triple Alpha rocess
Jovian Planets
inferior planets
Sc spiral galaxy
20. A volume of space where few - if any - galaxies are located
Ganymede (Jupiter)
matter dominated universe
Void
If it is in a denser medium - such as glass - it will move slower
21. Dark - reddish - low-pressure bands in Jupiter's atmosphere
belt
Red Giant
quasar
contrast northern lowlands and the southern highlands of mars...
22. The point where a superior planet is as far away from the sun as it can be (as seen from the Earth)
Ecliptic
Halo
opposition
Ole Roemer
23. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Gamma-ray Burst
If it is in a denser medium - such as glass - it will move slower
semimajor axis
Thermal Equilibrium
24. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Hubble law
widmanstatten pattern
Absolute Magnitude
SETI
25. How is the Hubble Law consistent with an expanding universe?
tectonics of Earth
Electromagnetic Radiation: Microwave
Electromagnetic Radiation: X-Ray
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.
26. 10^2 nm 10^7 nm
meteorite
Electromagnetic Radiation: Gamma Ray
We don't know. It might be but does not have to be.
protostar
27. Material that shoots rapidly out into space. Flares cause Auroras
terrestrial planet
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.
Flare
Meridian
28. The number of protons in an atom.
Electromagnetic Radiation: Ultraviolet Light
Electromagnetic Radiation: Microwave
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.
Atomic Number
29. The gap inthe outer portion of Saturn's A ring
Objective Lens
Light Gathering Power
Enke gap
cosmological principle
30. The amount of density needed to stop the universe from expanding and to begin the big crunch represented by Pc
greatest elongation
Secondary Mirror
critical density
Sa spiral galaxy
31. The normal eastward movement of a planet against the background of hte distant stars.
Atomic Number
Autumnal Equinox
Main Sequence
direct motion
32. Form honeycomb like patterns surrounding empty or nearly empty voids.
Molecular Clouds
MOONS: larger than mercury
superclusters
Radiative Diffusion
33. Any change in the speed or direction of an object's motion
cosmic singularity
blazar
acceleration
Ole Roemer
34. A small round distribution of gas surrounding a dying star
Planetary Nebula
terrestrial planet
Celestial Equator
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
35. All possible types of energy that can be emitted and absorbed by atoms.
Galilean satellite
rotation curve=winding dilemma?
Oort cloud
Electromagnetic Radiation
36. An empirical scheme for predictin ghe orbital distances of planets
Titus-Bode Law
Thermal Equilibrium
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.
CCD
37. In what chemical form are jupiters nitrogen - carbon and oxygen?
radio galaxy
differential rotation
Metals
Ammonia - methane - and water
38. The distance between a lens and its focal plane
Focal Length
Yes - frozen at the poles- remains protected from the suns rays
accretion disk
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
39. 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.
Heliocentric
Oort Cloud
open star clusters
Primary Mirror
40. The point where an inferior planet is as far away from the sun as it can be (as seen from the Earth)
Light: travels like a wave - detected like a particle
quarks
Population 1 vs Population 2 stars
greatest elongation
41. When particles are compressed to an unnatural state where their pressure is not related to their temperature
Globular Cluster
Milky way Galaxy
Planck time
Degeneracy
42. Is there water on the moon?
Precession
density waves
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
Yes - frozen at the poles- remains protected from the suns rays
43. The rock that makes up the lunar highlands
Ground State
Pulsar
Total Eclipse
anorthosite
44. The instant of time after the Big Bang when space and time obtained their characteristics. (t=10^-43 sec when gravity freezes out-instant when gravity started existing as a separate force)
Resolving Power
Planck time
Apollo asteroids
Light Curve
45. A galaxy emitting large amounts of energy at long wavelengths.
radio galaxy
Plague
differential rotation
Jupiters red spot
46. A logarithmically scaled value for the measured brightness of a star.
Vernal Equinox
cosmological principle
Apollo asteroids
Apparent Magnitude
47. The average distance between the Earth and the Sun (=1.5 x10^8km)
density parameter
Differential Rotation
Astronomical Unit
Meridian
48. A star that is burning hydrogen to helium in a shell surrounding it's core
H-are Diagram
MOONS: largest size
Red Giant Branch Star
Cosmic Microwave Background (CMB)
49. A telescope that uses lenses to focus light
Trojan asteroids
Refractor
general star population
most moons
50. A highly variable galaxy nucleus of which BL Lac is one. Their light is highly energetic and their spectra are featureless. (face on)
difference between maria and highlands of the moon.
blazar
Electromagnetic Radiation: Radio
White Dwarf