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Pre-Telescopic astronomy facts

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MONTEFALCON, Lady Cheyenne D.

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REVIEW 1-10Versión en línea Pre-Telescopic astronomy facts por MONTEFALCON, Lady Cheyenne D. 1 Which Greek philosopher argued Earth is spherical due to lunar eclipse shadows being round? a Isaac Newton b Pythagoras c Eratosthenes d Aristotle 2 How did Aristotle use stars to show Earth is round? a The Moon looks brighter at different places b Stars disappear at night c Some stars appear higher when you move south d The Sun changes color at different places 3 Eratosthenes measured a 7.2° shadow in Alexandria; distance to Syene was 5000 stadia. What did he calculate? a The diameter of the Moon b The speed of Earth’s rotation c The circumference of the Earth d The distance from Earth to the Sun 4 Which reasoning best explains Eratosthenes’ observation of different shadow angles in two cities shows Earth is curved? a Shadows form only in northern regions b Earth is flat but tilted toward the Sun c Different shadow angles at the same time indicate a curved surface between the cities d The Sun moves closer to one city 5 Which civilization made a 365-day calendar and watched Sirius to know when the Nile floods? a Early Chinese b Mayan c Ancient Egyptians d Polynesians 6 Why did ancient people watch the Sun’s yearly path in the sky? a To measure the speed of light b To calculate the distance to the Moon c To track seasons and agricultural activities d To predict volcanic eruptions 7 How did Polynesian sailors find direction at night? a Measuring the temperature of seawater b Observing the phases of the Moon only c Using the positions of stars as guides d Watching the movement of ocean waves 8 How does a solar eclipse happen? a The Moon moves between the Earth and the Sun, blocking sunlight b The Moon reflects more sunlight than usual c The Earth moves between the Sun and the Moon d The Earth moves farthest from the Sun 9 Why does retrograde motion happen in the Copernican model? a Earth moves faster than outer planets and appears to pass them b Planets stop moving temporarily in space c The Sun moves backward around the Earth d Epicycles cause planets to reverse direction 10 Planets move faster near the Sun and slower far away. Which law is this? a Kepler’s First Law b Law of Universal Gravitation c Kepler’s Third Law d Kepler’s Second Law Feedback 1 Aristotle argued the shadow on the Moon is round in lunar eclipses, indicating a spherical Earth. 2 Changing star altitudes with latitude suggested a curved surface. 3 Using angle and distance, he estimated Earth’s circumference. 4 If shadows differ at the same moment, surface curvature is implied. 5 Ancient Egyptians linked Sirius and Nile floods to calendar and agriculture. 6 Solar annual path helped farmers know planting and harvest times. 7 Stars served as celestial navigation guides for voyaging. 8 Solar eclipses occur when the Moon’s shadow falls on Earth. 9 As Earth overtakes outer planets, they seem to retrograde. 10 Planetary speed varies with area swept; faster near the Sun.

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REVIEW 1-10Versión en línea

por MONTEFALCON, Lady Cheyenne D.

Which Greek philosopher argued Earth is spherical due to lunar eclipse shadows being round?

How did Aristotle use stars to show Earth is round?

Eratosthenes measured a 7.2° shadow in Alexandria; distance to Syene was 5000 stadia. What did he calculate?

Which reasoning best explains Eratosthenes’ observation of different shadow angles in two cities shows Earth is curved?

Which civilization made a 365-day calendar and watched Sirius to know when the Nile floods?

Why did ancient people watch the Sun’s yearly path in the sky?

How did Polynesian sailors find direction at night?

How does a solar eclipse happen?

Why does retrograde motion happen in the Copernican model?

Planets move faster near the Sun and slower far away. Which law is this?

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