Q 01/05
A) Planetary motion
B) Electromagnetism
C) Chemical bonding
D) Thermodynamics
Answer · why
The three laws describe elliptical orbits, equal areas in equal times, and the link between period and distance.
Q 02/05
A) Tycho Brahe
B) Ole Rømer
C) Nicolaus Reimers
D) Christian Longomontanus
Answer · why
The two met at Benátky nad Jizerou in February 1600 and fell out within months before reconciling.
Q 03/05
A) Mercury
B) Jupiter
C) Venus
D) Mars
Answer · why
He never extended the analysis to other planets in Astronomia Nova because he had no calculating assistants.
Q 04/05
A) A perfect circle
B) An ellipse
C) A spiral
D) An egg-shaped ovoid
Answer · why
He had assumed it was too simple a solution for earlier astronomers to have missed.
Q 05/05
A) Equal arcs each month
B) Equal areas in equal times
C) Equal angles in equal times
D) Equal distances each day
Answer · why
He reached it geometrically after first proposing that a planet's speed was inversely proportional to its distance from the Sun.
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