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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 how an object resists accelerating when acted upon by a force. It is proportional the amount of matter in an object
greehouse effects
If it is in a denser medium - such as glass - it will move slower
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.
mass
2. The process responsible for creating the arms of flocculent spiral galaxies
radio galaxy
Self-Propogating Star Formation
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.
Wein's Law
3. Disk dust grains are made of all the elements that are not in gaseous form in space which blocks starlight and causes interstellar extinction
Differential Rotation
Electromagnetic Radiation: Visible Light
Radio Galaxy
interstellar dust
4. A spread of light with an uninterrupted wavelength distribution of energy.
Continuous Spectrum
Active Optics
matter dominated universe
greatest elongation
5. A word meaning 'the same everywhere throughout.'
Supernova (You can be my supernova girl)
Celestial Sphere
homogeneous
thinnest atmosphere
6. Jupiter
Supercluster
Objective Lens
Largest diameter
Cepheid variables
7. A plot of star absolute magnitude verses spectral type.
Focal Plane
H-are Diagram
radiation dominated universe
radio galaxy
8. A nearby galaxy with a quasar-like nucleus. closer but less bright than quasars-weaker
self-propagating star formation
Terrestrial Planets
Seyfert galaxy
cosmic fireball
9. When the Sun is farthest north of the celestial equator (about June 22)
Summer Solstice
Dwarf planets
dark matter
inferior planets
10. The mirror that determines the focus configuration of a reflector
condensation temperature
Dwarf planets
Secondary Mirror
Electron
11. Ganymede and Titan
chemical differentiation
resonance
Nebula
MOONS: larger than mercury
12. A push or a pull
Main Sequence Stars
Titus-Bode Law
Dark Matter
force
13. 1 mm 1μm
Make up of the terrestrial planets
How is winding dilemma solved?
Hyashi track
Electromagnetic Radiation: Infrared
14. 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
radio galaxy
aurora
Turn off Point
Dwarf planets
15. Venus (retrograde)
Cassegrain Focus
slowest rotation
Nucleus
Globular Cluster
16. The lowest energy of an atom.
Spectroscopic parallax
Ground State
Interstellar Extinction
Drake equation
17. Mercury and venus
Ground State
Quasar
fewest moons
Hubble law
18. The gap etween saturn's A and B rings
Horizontal Branch Star
supernova
Continuous Spectrum
Cassini division
19. A streak of light in the atmosphere
terrestrial planet
Annular Eclipse
radiant
meteor
20. The lens that gathers the light in a refractor
Objective Lens
molecular clouds
open star clusters
How is winding dilemma solved?
21. 1 mm 1μm
A family of radiant energy- includes light
radiation dominated universe
Umbra
Electromagnetic Radiation: Infrared
22. 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
mass
belt
Cepheid Variable
Cepheid variables
23. Ganymede and Titan
MOONS: larger than mercury
epicycle
scarp
Red Giant Branch Star
24. The state of having a balance between inflowing and outflowing heat-- the temp at every radial point is different but constant
Thermal Equilibrium
Turn off Point
E=mc2
Sa spiral galaxy
25. The point in its orbit where a planet is nearest the sun
Big Bang
Dwarf planets
Perihelion
coma
26. The class of all objects having high energy radiation coming from their nuclei. Active Galactic Nucleus- Blazars - Quasars - Radio and Emit synchrotron radiation
Eyepiece Lens
Population 1 vs Population 2 stars
AGN
comet
27. The rate of expansion of the universe.
Poor Cluster
Blackbody Curve
density parameter
Hubble constant
28. The rock that makes up the lunar highlands
Electron
Reflector
Color Index
anorthosite
29. Material that shoots rapidly out into space. Flares cause Auroras
highlands
Globular Cluster
Chandrasekhar Limit
Flare
30. A star that has become a red giant for the second and final time. It is burning helium to carbon in a shell surrounding the core
Olber's paradox
Asymptotic giant Branch Star
dark energy
Grand design spirals
31. A telescope that uses mirrors to focus light
great dark spots
difference between maria and highlands of the moon.
Open Cluster
Reflector
32. Moon in less than the angular diameter of the Sun.
Pulsar
Triple Alpha rocess
Annular Eclipse
hottest surface
33. A prominence seen against the disk of the sun
Apollo asteroids
contrast northern lowlands and the southern highlands of mars...
Active Optics
Filament
34. In Ptolemy's geocentric solar system - the small circle on which a planet moved.
AGN
density waves
epicycle
Drake equation
35. The surface of the sun
Photosphere
Synchrotron Rotation
asteroid
Wein's Law
36. The process responsible for creating the arms of flocculent spiral galaxies
Parallax
Self-Propogating Star Formation
widmanstatten pattern
molecular clouds
37. The apparent magnitude a star would have if it were at a distance of 10 parsecs.
Absolute Magnitude
Eyepiece Lens
Electron
chondrite
38. Elliptical orbits that come inside orbit of the Earth.
Continuous Spectrum
Apollo asteroids
Color Index
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.
39. Mercury
thinnest atmosphere
Turn off Point
scarp
Milky way Galaxy
40. The displacement of spectral lines to redder colors caused by the expansion of the universe.
Positive - Converge - Greater than 1
Metals
Thermonuclear Fusion
cosmological red shift
41. A term referring to the orbital character of stars near the Sun
MOONS: thickest atmosphere
least dense
Triple Alpha rocess
Differential Rotation
42. The mix of pure photon energy that emerged at the start of the universe.
Bulge
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.
Planetary Nebula
cosmic fireball
43. 30AU to 50Au from sun - consists of ancietn premordial objects made of frozen ice and dust-35000 objects or more that are larger than 100 km in diameter and many more smaller than this
Kuiper belt
slowest rotation
Most dense
Black Hole
44. The average distance between the Earth and the Sun (=1.5 x10^8km)
Apollo asteroids
Astronomical Unit
Ole Roemer
Plank's Law
45. The law that predicts the possible types of spectra.
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46. Saying that the sky should not get dark at night because all lines of sight end on a star meaning that the night sky should be ablaze BUT the big bang - because the universe had a beginning - says that the sky gets dark because out in space - galaxie
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47. A faint - remarkably uniform distribution of radiation in space
meteor shower
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
Cosmic Microwave Background
Population 1 vs Population 2 stars
48. The elementary building blocks from which protons and neutrons are formed.
quarks
3 reasons we orbit satellites to observe universe
Instability strip
Convection
49. Relativity predicts that nothing can travel faster than the speed of light in a vacuum - How can it move slower?
smallest diameter
Asymptotic giant Branch Star
If it is in a denser medium - such as glass - it will move slower
Limb darkening
50. Form honeycomb like patterns surrounding empty or nearly empty voids.
Flat - Flat
We don't know. It might be but does not have to be.
Triple Alpha rocess
superclusters