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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. Where is the center of the expansion
Refractor
radio galaxy
matter dominated universe
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.
2. Light scattered through the atmosphere that degrades astronomical images
Light Pollution
Thermal Equilibrium
isotropic
Heliocentric
3. The north-south line passing directly overhead through the zenith.
terrestrial planet
Meridian
Instability strip
neutrino
4. A perfect absorber and radiator of electromagnetic radiation.
weight
comet
Blackbody
Triple Alpha rocess
5. A very low mass particle formed in solar fusion reactions that reacts only weakly with matter
neutrino
Cassini division
Positive - Converge - Greater than 1
quasar
6. Radiation (possibly left over from the big bang) that fills the universe. Perfect black body spectrum and tells us a bit aout how galaxies are formed.
supernova
greatest elongation
Cosmic Microwave Background (CMB)
White Dwarf
7. Jupiter
AGN
Absorption Spectrum
fastest rotation
Drake equation
8. Any class of objects with a uniform luminosity used to determine distance.
standard candle
terrestrial planet
Interstellar Extinction
Galilean satellite
9. VENUS
Sa spiral galaxy
Celestial Sphere
widmanstatten pattern
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
10. Distribution of dust (tells us disk is thin) - find distances to O&B stars and H2 regions (arms are sights of star formation and OB stars live and die at location of birth) -Milky way has four arms. Sun is in spur apart from arms.
mapping the structure of Milky Way disk
comet
Plank's Law
inferior planets
11. Electromagnetic Radiation
Filament
Color Index
A family of radiant energy- includes light
Oort Cloud
12. Sulfurous volcanoes - pools of liquid sulfur - surface resembles cheese pizza ACTIVE SURFACE
retrograde motion
mass
Io (jupiters moon)
Winter Solstice
13. The mirror that gathers the light in a reflector
Primary Mirror
Parsec
Flat - Remain Parallel - Exactly 1
shape and color of SPIRAL galaxies
14. When material is heated and moves taking the heat energy with it
dark matter
Convection
Parallax
Electromagnetic Radiation: Radio
15. The place in the sky that the Earth's axis points toward (can be either north or south)
Positive - Converge - Greater than 1
Colestial Pole
Red Giant
Interstellar Extinction
16. What is the universe expanding into?
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.
Halo
CMB
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.
17. When a planet lines up with the sun inthe sky
Spectral Lines
300000 KM/sec
Eyepiece Lens
conjunction
18. An important quality of telescopes that increases as the square of the primary mirror or objective lens
Light Gathering Power
High Velocity Stars
Focal Plane
Cepheid Variable
19. Material that shoots rapidly out into space. Flares cause Auroras
Jupiters red spot
Flare
synchronous rotation
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.
20. A spherical shell of comets that orbit the sun at a great distance (roughly two light years from the sun)
Terrestrial Planets
Oort cloud
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.
2 Reasons Why there are Supermassive Black holes at the center of every Galaxy
21. A small round distribution of gas surrounding a dying star
Planetary Nebula
tectonics of Earth
Hubble law
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.
22. The organization of clusters of galaxies into sheets and strings
Doppler Shift
Supercluster
Astronomical Unit
semimajor axis
23. A representation of the changes in color and brightness of an evolving protostar.
density parameter
Hyashi track
density waves
Sunspot cycle
24. The measure of a variable star's apparent magnitude as it brightens and dims with time
Light Curve
Io (jupiters moon)
Big Crunch
Nucleus
25. 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
26. A small and dim but hot star.
great red spot
Celestial Equator
Interstellar Extinction
White Dwarf
27. The distance a moon can be from a planet before shattering from tidal forces
Parallax
Eyepiece Lens
Hubble law
roche limit
28. The layer of the sun just above the photosphere
great dark spots
Chromosphere
Gravitational Lens
Proton-proton chain
29. Venus (retrograde)
Winter Solstice
slowest rotation
radio lobe
Olber's paradox
30. Largest moon in solar system - two differenet types of terrain - darker terrain is older - NOT ACTIVE SURFACE
Enke gap
inferior planets
CMB
Ganymede (Jupiter)
31. Loops that trace the magnetic field as it erupts from a sunspot area and arches over to an adjacent area. They glow in the light of gas pouring out of corona and falling into photosphere.
cosmological red shift
Secondary Mirror
Coronal Loop
deferent
32. The telescope configuration that has the focus placed at the back of the primary mirror
Cassegrain Focus
Hubble constant
Neutron Star
Light Gathering Power
33. Small moons that maintain the shape of rings around Saturn and Uranus
tectonics of Venus
Light-Year
Shepherd satellite
Granules
34. The part of the Milky way that has on-going star formation
Disk
comet
Seyfert galaxy
Black Hole
35. The opaque universe that existed for 300000 years after the Big Bang. (photons outnumbered nuclei by 1 billion to one - so less light)
Light: travels like a wave - detected like a particle
Instability strip
A family of radiant energy- includes light
radiation dominated universe
36. Why does the earth have few craters while the moon has many?
Earth resurfaces itself due to erosion and plate tectonics - while the moon has neither.
belt
fastest 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
37. A younger cluster of stars - found in the galaxy disk
Rich vs poor clusters
Differential Rotation
Open Cluster
Olber's paradox
38. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
Red Giant
epicycle
chondrite
Planetary Nebula
39. What causes the zones and belts on jupiter and saturn?
Umbra
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
H2 Regions
isotropic
40. An object that may remain after a star explodes
Interstellar Extinction
Oort cloud
Wein's Law
Neutron Star
41. 1μm 100 nm
accretion
Blackbody
Synodic Day
Electromagnetic Radiation: Visible Light
42. 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)
Planck time
Neutron Star
Terrestrial Planets
Rich vs poor clusters
43. A very dense - highly populated cluster of galaxies
Kirkwood gaps
Apparent Magnitude
Total Eclipse
Rich Cluster
44. Venus
accretion disk
Thermonuclear Fusion
Roundest orbit
Zenith
45. Venus
Photometry
Radiative Diffusion
Roundest orbit
Europa (Jupiters moon)
46. A term referring to Earth-like planets
Bulge
Convection
terrestrial planet
Nebula
47. A fusion process in which a carbon atom transmutes to oxygen and back - creating a helium atom in the process
Winter Solstice
Granules
CNO Cycle
Perihelion
48. The family of radiant energy that includes light as a subset
Active Optics
Electromagnetic Radiation
Blackbody Curve
Blackbody Curve
49. The average distance between the Earth and the Sun (=1.5 x10^8km)
Astronomical Unit
Galilean satellite
Cepheid variables
greehouse effects
50. Small bulges - loosely wound - massive arms - arms have many H2 regions and look very lumpy
protostar
Interstellar Extinction
Sc spiral galaxy
Eyepiece Lens