Stars, Galaxies & Spaceflight
Beyond the planets: stars, distance and getting off the ground.
Which galaxy contains our Solar System?
Most of what we know about the universe arrived through instruments, and the instruments shape what we can know.
Astronomy is limited by what can be detected. For most of its history that meant visible light, which is a narrow slice of what the universe emits, and every extension into another part of the spectrum has produced discoveries nobody predicted. These questions cover how telescopes work, why they are placed where they are, and what different instruments are actually detecting — including several that collect no light at all.
Every question in this quiz is listed below with its correct answer and the reasoning behind it. Play first if you would rather not see the answers — or read through as a study sheet.
Play it insteadAnswer: B. Lenses
Why: Reflectors use mirrors instead, which is what almost all large modern telescopes do because big mirrors are easier to support than big lenses.
Answer: A. Thinner, steadier, drier air above them
Why: Atmospheric turbulence blurs images, so height, dry air and distance from city lights all help. Altitude gets you above a good share of the water vapour.
Answer: D. Radio waves emitted by objects in space
Why: They can operate in daylight and through cloud, and they revealed pulsars and the cosmic microwave background.
Answer: C. The atmosphere blocks and blurs much of the spectrum
Why: X-rays and much infrared never reach the ground at all, so those instruments have to be above the atmosphere to work.
Answer: B. Deep underground or under ice
Why: Rock or ice filters out other particles, leaving neutrinos, which pass through almost everything and interact very rarely.
Answer: A. Deforming a mirror many times a second to cancel atmospheric blur
Why: A reference star, sometimes an artificial one created with a laser, is used to measure the distortion in real time.
Answer: D. The resolving power of a much larger instrument
Why: Linking dishes across continents is how the first image of a black hole's shadow was produced.
Answer: C. As it was when the light left it
Why: Looking further away is therefore looking further back in time, which is how the early universe can be observed at all.
Answer: B. Composition, temperature and motion of distant objects
Why: Splitting light reveals absorption lines, and their shift toward red or blue shows whether an object is moving away or toward us.
Answer: A. From many hexagonal segments acting as one
Why: Segments can be made, transported and aligned individually. A single mirror beyond about eight metres begins to sag under its own weight.
Everything overhead is a clue about distance, time and scale. How to read a dark sky without a telescope.
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Beyond the planets: stars, distance and getting off the ground.
Which galaxy contains our Solar System?
Ten questions on the eight planets, from the hottest surface to the one lying on its side.
Which planet orbits closest to the Sun?
Phases, tides, the far side and the slow retreat — ten questions on the nearest thing in the sky.
What causes the phases of the Moon?