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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. 1-orbit aroudn the sun 2- are in hydrostatic equilibrium and 'mostly round' 3- have not cleared debris around its orbit 4- are not satellites
Electromagnetic Radiation: Ultraviolet Light
Occam's razor
Astronomical Unit
Dwarf planets
2. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
slowest rotation
Flat - Flat
Granules
If it is in a denser medium - such as glass - it will move slower
3. 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)
Main Sequence
Planck time
chemical differentiation
Blackbody Curve
4. The north-south line passing directly overhead through the zenith.
Meridian
Horizontal Branch Star
gravity
Electromagnetic Radiation: Microwave
5. A spectrum of light with energy at only a few wavelengths.
Emission Spectrum
Cosmic Microwave Background
resonance
HII Region
6. Comglomerates of ice and rock that orbit the sun in highly elliptical paths
Halo
great dark spots
comet
Make up of the terrestrial planets
7. The part of the Milky way that has on-going star formation
rotation curve=winding dilemma?
Flat - Remain Parallel - Exactly 1
Disk
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
8. A logarithmically scaled value for the measured brightness of a star.
comet
Apparent Magnitude
Eyepiece Lens
planetary nebula
9. A subatomic particle with a negative charge. It creates light.
Filament
Geocentric
Electron
aurora
10. Venus
Roundest orbit
Red Giant Branch Star
density
Planck time
11. The mass of an object divided by its volume
Jupiters red spot
Electromagnetic Radiation: X-Ray
density
Kirchhoff's Law
12. A method of finding a star's distance from its absolute magnitude and spectral type or color.
Spectroscopic Parallax
Thermal Equilibrium
Primary Mirror
Sidereal Day
13. The fate of the universe if it is closed. The universe expanding as much as possible and then retracting
Photometry
Oort cloud
MOONS: roundest shape
Big Crunch
14. Why do Galaxies move very rapidly in the interiors of the dense clusters?
Meridian
Light Pollution
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.
Dark matter is located at center of clusters - pulling the cluster members into faster orbits--dark matter gravity keeps objects in galxies bound.
15. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
acceleration
interstellar dust
reflection star clusters
radiation dominated universe
16. A streak of light in the atmosphere
meteor
MOONS: largest size
Gamma-ray Burst
shape and color of ELLIPTICAL galaxies
17. An evolved star - past the helium flash that is burning helium to carbon in it's cores
quarks
aphelion
Celestial Equator
Horizontal Branch Star
18. In what chemical form are jupiters nitrogen - carbon and oxygen?
Spectral Lines
neutrino
Ammonia - methane - and water
CCD
19. A force exerted by reflecting sunlight
Parallax
Cosmological Principle
radiation pressure
self-propagating star formation
20. A very distant - star-like object with huge - broad emission lines. Probably the nucleus of a distant active galaxy.
resonance
Particle Horizon
highlands
quasar
21. A term referring to the orbital character of stars near the Sun
Differential Rotation
radiation dominated universe
Electromagnetic Radiation: Radio
aurora
22. A push or a pull
Oort Cloud
force
Disk
inferior planets
23. The fusion process that turns three helium nuclei into a carbon nucleus
zone
Kirchhoff's Law
Photon
Triple Alpha rocess
24. A huge sphere of tenuous gas surrounding the nucleus of a comet
Yes - frozen at the poles- remains protected from the suns rays
Gravitational Lens
Light: travels like a wave - detected like a particle
coma
25. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
zone
Oort cloud
Largest diameter
26. Collections of young - hot stars
Rich Cluster
OB Associations
Make up of the jovian planets
Photometry
27. The law that syas light energy from a blackbody increases as (temperature^4)
Magnification
Stephen-Boltzman Law
Interstellar Extinction
Objective Lens
28. Venus (retrograde)
resonance
slowest rotation
Proton-proton chain
High Velocity Stars
29. The cosmological principle is the assumption that the universe is isotropic and homogeneous.The Big Bang assumes it to be a correct principle so that what we observe is exactly like What is too far away to be observed.
Triple Alpha rocess
Cosmological Principle
Secondary Mirror
most eccentric orbit
30. The universe is isotropic - homogeneous - and without beginning or end in time and space. If the universe is truly homogeneous then every line of sight will eventually end on a galaxy. If it has existed forever then there has been enough time for lig
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183
31. Medium bulge - moderately would arms - arms have H2 regions in them and look sort of lumpy
If it is in a denser medium - such as glass - it will move slower
Sb spiral galaxy
Quasar
matter dominated universe
32. A distance measure determined by the shifting of a star against the background sky every 6 months.
density waves
Light Pollution
open star clusters
Parsec
33. Electromagnetic Radiation
A family of radiant energy- includes light
shape and color of SPIRAL galaxies
Sc spiral galaxy
Reflector
34. All wavelengths of light emitted by a blackbody.
MOONS: largest size
reflection star clusters
Blackbody Curve
hottest surface
35. A rock or iron specimen that has fallen from space
partile horizon
meteorite
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
partile horizon
36. A spinning neutron star
Pulsar
opposition
Trojan asteroids
cosmology
37. The gap inthe outer portion of Saturn's A ring
Ammonia - methane - and water
Enke gap
meteor shower
Black Hole
38. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
rotation curve = dark matter?
Lagrangian Razor
Open - flat - and closed.
Seyfert galaxy
39. A measure of the seasonal shifting of a star's position against farther stars or galaxies. The closer the star - the greater is the angular distance it shifts. We use it to find distances to stars that are up to 1000 pc away.
Terrestrial Planets
most moons
Parallax
Colestial Pole
40. An evolved star - past the helium flash that is burning helium to carbon in it's cores
hottest surface
Horizontal Branch Star
regolith
Superior planets
41. Saturn
MOONS: most geologically active
Neutron Star
epicycle
least dense
42. Milky way galaxy is a member - a small poor cluster-about 30 galaxies
Colestial Pole
Ole Roemer
The Local Group
Sa spiral galaxy
43. The sinking of denser elements to the center of a young molten planet
Milky way Galaxy
mare basalt
Nucleus
chemical differentiation
44. Mercury
Electromagnetic Radiation: Gamma Ray
smallest diameter
Radio Galaxy
accretion disk
45. A fusion process in which protons build together to form helium
Drake equation
matter dominated universe
era of recombination
Proton-proton chain
46. A galaxy sending out a stream of material from its nucleus
Radio Galaxy
Globular Cluster
Triple Alpha rocess
AGN
47. When material is heated and moves taking the heat energy with it
deferent
Convection
Globular Cluster
Superior planets
48. Latin for 'cloud'. A word used to describe the collections of gas and dust in the Milky Way and other galaxies
reflection star clusters
Halo
Nebula
Thermal Equilibrium
49. What Ole Roemer used to measure the speed of light in a vacuum
Gamma ray bursts
Eclipses of the Moons of Jupiter
superclusters
Brown dwarf
50. The equation that describes how matter equates with energy
Astronomical Unit
accretion disk
E=mc2
Wein's Law