Origins of Astronomy Flashcards
Q0Q1. The national observatory south of Penticton studies the Universe in what part of the electromagnetic spectrum?
(a) Visible.
(b) Ultraviolet.
(c) Infrared.
(d) Radio.
(d) Radio.
Q0Q2. The Sun releases the majority of its light energy in what part of the electromagnetic spectrum? (a) Visible.
(b) Ultraviolet.
(c) Infrared.
(d) Radio.
(a) Visible.
Q0Q3. The average Earth-Sun distance is
(a) 384,400 km.
(b) 150,000,000 km.
(c) 4.50 billion km.
(d) 9.46 trillion km.
(b) 150,000,000 km.
Q0Q4. What percentage of the Solar System’s mass is in the Sun?
(a) 90%.
(b) 99%.
(c) 99.8%.
(d) 100%.
(c) 99.8%.
Q0Q5. The next closest star after the Sun, Proxima Centauri, is approximately
(a) 150,000,000 km from Earth.
(b) 39,700,000,000,000 km from Earth.
(c) 10 light-years from Earth.
(d) 26,000 light-years from Earth.
(b) 39,700,000,000,000 km from Earth.
Q0Q6. The Milky Way galaxy has a diameter of approximately
(a) 4.2 light-years.
(b) 26,000 light-years.
(c) 100,000 light-years.
(d) 2.5 million light-years.
(c) 100,000 light-years.
Q0Q7. The Local Group of Galaxies is dominated by the Milky Way and which other galaxy?
(a) Large Magellanic Cloud.
(b) Triangulum.
(c) Andromeda.
(d) M87.
(c) Andromeda.
Q0Q8. What is the approximate age of the Universe?
(a) 13.8 billion years.
(b) 4.6 billion years.
(c) 6000 years.
(d) We don’t know.
(a) 13.8 billion years.
Q1Q1. The stone array affectionately known as Pen Henge in Penticton tracks the position of the setting Sun using a heel stone and three stone markers. On the winter solstice, the Sun will set directly over the marker that sits
(a) due west of the heel stone.
(b) northwest of the heel stone.
(c) southwest of the heel stone.
(d) due south of the heel stone.
(c) southwest of the heel stone.
Q1Q2. Approximately how many hours of daylight do we get in Kelowna on the winter solstice?
(a) 4 hours.
(b) 8 hours.
(c) 12 hours.
(d) 16 hours.
(b) 8 hours.
Q1Q3. What is the approximate altitude of the Sun at local noon today as viewed from Kelowna?
(a) 64°.
(b) 17°.
(c) 20°.
(d) 41°.
(c) 20°.
Q1Q4. What is the approximate altitude of the Sun at local noon on the vernal (spring) equinox as viewed from Kelowna?
(a) 17°.
(b) 20°.
(c) 41°.
(d) 64°.
(c) 41°.
Q1Q5. In which month does the “emu in the sky” appear directly overhead at midnight as viewed from Sydney, Australia?
(a) February.
(b) May.
(c) August.
(d) November.
(b) May.
Q1Q6. Which ancient civilization used the stars to successfully navigate the seas at night?
(a) Polynesians.
(b) Chinese.
(c) Early British.
(d) Mayans.
(a) Polynesians.
Q1Q7. The daily reports of this civilization’s “sky watchers” represent the longest continuous astronomical record.
(a) Chinese.
(b) Early British.
(c) Egyptians.
(d) Mayans.
(a) Chinese.
Q1Q8. Astrology set the foundation for astronomy by
(a) producing detailed star maps.
(b) introducing number systems.
(c) developing arithmetic and basic algebra.
(d) All of the above.
(d) All of the above.
Q1Q9. Which ancient civilization used a base-20 number system to study the motions they observed in the sky?
(a) Mayans.
(b) Babylonians.
(c) Egyptians.
(d) Chinese.
(a) Mayans.
Q1Q10. In which zodiac constellation will the Sun appear on the vernal equinox in 2019?
(a) Aries.
(b) Pisces.
(c) Aquarius.
(d) Taurus.
(b) Pisces.
Q2Q1. What is the approximate altitude of the Sun at local noon today(January 15th) as viewed from Kelowna?
(a) 41°.
(b) 21°.
(c) 20°.
(d) 17°.
(b) 21°.
Q2Q2. One year is
(a) exactly 365 days.
(b) the time it takes to go from vernal equinox to vernal equinox.
(c) the time it takes for the Earth go once around the Sun.
(d) Both b and c.
(b) the time it takes to go from vernal equinox to vernal equinox.
Q2Q3. Precession (“wobble”) of the Earth’s spin axis completes one cycle every
(a) 23 hours, 56 minutes.
(b) 365.24219 days.
(c) ~26,000 years.
(d) ~2200 years.
(c) ~26,000 years.
Q2Q4. In which zodiac constellation did the Sun appear on the vernal equinox in 500 BC?
(a) Aries.
(b) Pisces.
(c) Aquarius.
(d) Taurus.
(a) Aries.
Q2Q5. If the Earth’s spin axis were inclined 40° relative to a perpendicular to the Earth’s orbital plane, then the seasons would be
(a) less severe than what we currently experience.
(b) more severe than what we currently experience.
(c) almost non-existent (i.e., we would experience no seasons).
(d) unchanged from what we currently experience, since the tilt of the Earth’s axis has no effect on the seasons
(b) more severe than what we currently experience.
Q2Q6. Ryan took the picture below during the onset of the lunar eclipse on Sunday. The Moon was about 35° above the horizon in the east.
(a) a sphere.
(b) flat, but with a circular cross-section.
(c) Either b or c.
(d) The shape of the Earth cannot be determined using its (twodimensional) shadow.
(a) a sphere.
Q2Q7. Which of the following natural philosophers presented the first known Universe (or “World”) model?
(a) Thales.
(b) Anaximander.
(c) Democritus.
(d) Aristotle.
(b) Anaximander.
Q2Q8. Who was the first to successfully measure the circumference of the Earth?
(a) Pythagoras.
(b) Eratosthenes.
(c) Thales.
(d) Anaximander.
(b) Eratosthenes.
Q2Q9. Which of the following natural philosophers suggested that all things are composed of “atoms”?
(a) Thales.
(b) Aristotle.
(c) Democritus.
(d) Archimedes.
(c) Democritus.
Q2Q10. The fastest motion in the sky is the
(a) prograde (eastward) motion of the planet Mercury relative to the stars.
(b) retrograde (westward) motion of the planet Mars relative to the stars.
(c) westward daily motion of the Sun, Moon, planets, and stars.
(d) eastward motion of the Moon relative to the stars.
(c) westward daily motion of the Sun, Moon, planets, and stars.
Q3Q1. What is the approximate altitude of the Sun at local noon today (Jan 29) as viewed from Kelowna? (a) 23°.
(b) 21°.
(c) 17°.
(d) 41°.
(a) 23°.
Q3Q2. The following is a schematic representation of Aristotle’s (qualitative) geocentric model. This model does not explain
(a) the daily motion of the Sun, Moon, planets, and stars.
(b) the retrograde motion of the planets relative to the stars.
(c) the non-uniform motion of the Sun, Moon, and planets relative to the stars.
(d) Both b and c.
(d) Both b and c.
Q3Q3. Aristarchus (in ~270 BC) estimated the Sun’s diameter to be approximately
(a) 7 times that of the Earth.
(b) 109 times that of the Earth.
(c) 3 times that of the Earth.
(d) 19 times that of the Earth.
(a) 7 times that of the Earth.
Q3Q4. Who was the first to successfully measure the distance between the Earth and the Moon?
(a) Eratosthenes.
(b) Aristarchus.
(c) Hipparchus.
(d) Ptolemy.
(c) Hipparchus.
Q3Q5. Which ancient Greek measured the length of the year to within 7 minutes?
(a) Hipparchus.
(b) Aristarchus.
(c) Ptolemy.
(d) Pythagoras.
(a) Hipparchus.
Q3Q6. Who first suggested using epicycles to explain the retrograde motion of the planets?
(a) Aristotle.
(b) Ptolemy.
(c) Archimedes.
(d) Apollonius.
(d) Apollonius.
Q3Q7. The following is a schematic representation of the geocentric model including epicycles.To what object does the arrow point?(5th element above the earth)
(a) Sun.
(b) Mercury.
(c) Mars.
(d) Venus.
(d) Venus.
Q3Q8. What did Ptolemy do to explain the non-uniform motion of the Sun, Moon, and planets relative to the stars?
(a) He used a prime mover.
(b) He used epicycles on deferents.
(c) He offset the center of each circular deferent from the center of the Earth.
(d) Both b and c.
(c) He offset the center of each circular deferent from the center of the Earth.
Q3Q9. In approximately what year did Ptolemy publish Mathematique Syntaxis (the “Almagest”)?
(a) 150 AD.
(b) 350 AD.
(c) 150 BC.
(d) 350 BC.
(a) 150 AD.
Q3Q10. What did Ptolemy estimate to be the radius of the Universe (i.e., the distance from the center of the Earth to the sphere of the stars)?
(a) 150 million km.
(b) 120 million km.
(c) 59 Earth radii.
(d) 40,000 km.
(b) 120 million km.
Q11Q1. The Millennium Simulation (released in 2005) shows
(a) the futures of the Milky Way and Andromeda.
(b) galaxies at the edge of the ‘visible’ Universe.
(c) the large-scale structure of the present-day Universe.
(d) the Universe within 200 million light-years of the Milky Way
(c) the large-scale structure of the present-day Universe.
Q11Q2. The Hubble Ultra Deep Field (imaged in 2009) shows
(a) the futures of the Milky Way and Andromeda.
(b) galaxies at the edge of the ‘visible’ Universe.
(c) the large-scale structure of the present-day Universe.
(d) the Universe within 200 million light-years of the Milky Way.
(b) galaxies at the edge of the ‘visible’ Universe.
Q11Q3. The ratio of dark matter to luminous matter on galaxy-cluster scales is approximately
(a) 2:1.
(b) 3:1.
(c) 5:1.
(d) 10:1.
(c) 5:1.
Q11Q4. Einstein’s general theory of relativity describes gravity as
(a) an invisible attraction between masses.
(b) a striving of the earth element within an object to reach the Earth.
(c) curved space.
(d) an exchange of force carriers called gravitons.
(c) curved space.
Q11Q5. The gravitational center of the Milky Way is occupied by a
(a) globular star cluster.
(b) supermassive black hole.
(c) quasar.
(d) Both b and c.
(b) supermassive black hole.
Q11Q6. The present-day Universe is
(a) expanding, but faster than it was ~7 billion years ago.
(b) expanding, but slower than it was ~7 billion years ago.
(c) contracting, due to the mutual gravitation of all the mass/energy in the Universe.
(d) static (i.e., neither expanding nor contracting).
(a) expanding, but faster than it was ~7 billion years ago.
Q11Q7. Dark energy is required to explain
(a) the acceleration of the expansion of the Universe. (b) the expansion of the Universe.
(c) why stars, gas, and dust in the middle and outer parts of galaxies move as fast as they do.
(d) the origin of the Universe.
(a) the acceleration of the expansion of the Universe.
Q11Q8. Dark energy makes up what percentage of the present-day mass/energy content of the Universe? (a) 90%.
(b) 24%.
(c) 5%.
(d) 71%.
(d) 71%.
Q11Q9. The best current estimate for the age of the Universe is
(a) 13.82 billion years.
(b) 13.73 billion years.
(c) 4.56 billion years.
(d) We don’t know how old the Universe is.
(a) 13.82 billion years.
Q11Q10. The Cosmic Microwave Background (CMB) radiation was ‘released’ when the
(a) Universe first formed hydrogen and helium nuclei. (b) Universe first formed hydrogen and helium atoms. (c) Universe was a ‘soup’ of charged particles.
(d) first stars were formed in the Universe.
(b) Universe first formed hydrogen and helium atoms.
Q10Q1. Who used globular clusters to show that the Sun is not near the center of the Milky Way?
(a) William Herschel.
(b) Jacobus Kapteyn.
(c) Harlow Shapley.
(d) Edwin Hubble.
(c) Harlow Shapley.
Q10Q2. Cepheid variable stars are used as indirect distance estimators. Which of the following best explains how this is done?
(a) Cepheid variables all have the same luminosity. We use this luminosity and the apparent brightness to solve for distance via L = b·4πd2.
(b) Cepheid variables have two different luminosities. We use the spectral type to determine which luminosity the Cepheid has, and then use this luminosity and the apparent brightness to solve for distance via L = b·4πd2.
(c) Cepheid variables have measurable pulsation periods which are physically related to luminosity. We use the pulsation period to estimate luminosity, and then use this luminosity and the apparent brightness to solve for distance via L = b·4πd2.
(d) When Cepheid variables explode as supernovae, they always reach the same peak luminosity. We use the peak luminosity of the supernova and apparent brightness to solve for distance via L = b·4πd2.
(c) Cepheid variables have measurable pulsation periods which are physically related to luminosity. We use the pulsation period to estimate luminosity, and then use this luminosity and the apparent brightness to solve for distance via L = b·4πd2.
Q10Q3. The present-day distance uncertainty for Cepheid variables is
(a) better than 1%.
(b) ~5%.
(c) ~10%.
(d) 20‒50%.
(c) ~10%.
Q10Q4. During the Great Debate in 1920, Heber Curtis argued that
(a) globular clusters are located beyond the Milky Way’s halo.
(b) spiral nebulae are “island universes” outside the Milky Way’s halo.
(c) spiral nebulae are located within the Milky Way’s halo.
(d) the Milky Way is too big for there to be anything beyond it.
(b) spiral nebulae are “island universes” outside the Milky Way’s halo.