Question 1 of 10

Astronauts orbiting Earth aboard the International Space Station feel weightless as they experience microgravity. Do you experience gravity walking around Earth?

  • Only objects newly entering Earth’s atmosphere experience gravity.
  • Only when pulled back to Earth after jumping.
  • Only when you jump up.
  • Yes, about 1G.

    That’s right! Gravity may be the weakest of the four fundamental forces, but it’s still strong enough to keep you tethered to Earth! Even though you don’t consciously feel the pull of Earth’s gravity in daily life, you are subject to it.

Question 2 of 10

In 2006, the International Astronomical Union voted to revoke Pluto’s status as one of the classic planets of the solar system. Which definition of “planet” do some planetary scientists still push for that would reinstate Pluto’s status as a planet?

  • The object has to orbit the sun.
  • It has to have at least one moon, proving that it can pull objects into its orbit.
  • It has to be massive enough to assume hydrostatic equilibrium, which is a fancy way to say that it needs to be round.

    Nice one! According to this definition, Earth’s moon and many other moons would also be planets.

  • The object has to “clear the neighborhood” around itself, meaning it has to have a strong enough gravitational pull that there aren’t things like asteroids or comets left in the path of its orbit.

Question 3 of 10

How is a star born?

  • White holes spit out material that eventually combines to spit out a star.
  • Asteroids and other objects collide, and they leave behind the basic components of stars.
  • Black holes spit out star fragments, and eventually enough of them build up to form a star.
  • Clouds of dust and gas reach a critical mass, collapse under their own gravity and then continue to accumulate more material.

    Perfection! This accumulation can happen for many reasons: because of random fluctuations of density within the cloud of dust and gas or because of an external influence like a collision with another molecular cloud, a supernova or even other stars forming close by.

Question 4 of 10

Liu Cixin’s novel, The Three-Body Problem, was recently turned into a hit Netflix show by the same name. The three-body problem is a real physics concept — and so is the star system that is referenced in the TV series. Which star system is that?

  • The Goldilocks zone
  • Alpha Centauri

    You got it! At 4.2 to 4.4 light-years from Earth, the Alpha Centauri system is our closest neighboring star system. It comprises three stars: Alpha Centauri A, B and C. Alpha Centauri C, often called Proxima Centauri, is orbited by a small, rocky exoplanet that some scientists think could be habitable. We don’t know much about it yet, since our telescopes aren’t powerful enough to image it.

  • Tatooine
  • UHZ1

Question 5 of 10

The majority of matter in the universe isn’t observable matter, like you or me or the device that you’re reading this on. It’s DARK matter — which seemingly doesn’t interact with normal matter! How much of the universe is made up of normal matter?

  • 4% to 5%

    You got it, dude! Even though normal matter makes up everything we see in the universe, scientists believe that there must be more than five times as much dark matter as normal matter hanging around to fit their observations.

  • 10% to 12%
  • 25% to 27%
  • 1% to 2%

Question 6 of 10

The universe is expanding — and it’s accelerating as it expands. Scientists call the force driving that accelerating expansion dark energy, and they measure it with cosmic probes. What’s one example of a cosmic probe?

  • Exoplanets, like Proxima Centauri b
  • Human-made satellites, like Sputnik and Explorer
  • Supernovas — exploding stars

    Stellar (no, literally)! Scientists use many things to measure dark energy — supernovas, the distribution of galaxies and the cosmic microwave background, to name just a few. Cosmologist Brian Nord likens these probes’ movement in space-time to buoys in the ocean: As we look at their movement over time, we learn more about how space-time is expanding.

  • Radio antennae built in remote locations on Earth

Question 7 of 10

Astronauts can face multiple health hazards while living in space. On the list below, which is NOT a risk presented by spaceflight to the human body?

  • Increased radiation exposure due to solar storms and cosmic rays
  • Weakened muscles and bone density due to microgravity
  • Weakened immune system due to the hostile, closed environment
  • Disruption to the body’s aging process due to time dilation

    Correct! While time dilation is a real principle of physics that affects astronauts, its effects on the human body in orbit would be minimal. The five primary hazards of human spaceflight, according to NASA, are space radiation, isolation and confinement, distance from Earth, gravity (and the lack of it) and closed or hostile environments.

Question 8 of 10

If you fell headfirst into a stellar-mass black hole, astrophysicist Priyamvada Natarajan says, the difference in the strength of gravity between your hair and the tips of your toes would be so strong that it would rip you apart — yikes! What’s the technical term for that?

  • Tendonosis
  • Spaghettification

    Oh, the pasta-bilities! As you approached a black hole (theoretically, we’re hoping), you’d be stretched in the direction of the black hole and compressed perpendicular to it, making you a long, noodle-y shape. And while we haven’t observed this happening to humans, researchers have observed the spaghettification of stars.

  • Extensibility
  • Expoliation

Question 9 of 10

In 1964, two radio astronomers in New Jersey were trying to track satellite signals when they picked up a strange hum — one that could be heard everywhere they pointed their antenna. What did that hum turn out to be?

  • The office microwave, which was emitting residual electromagnetic waves
  • Noise pollution coming from New York City, just across the river
  • Low-level background radiation, left over from the big bang

    Yep! Even though scientists Arno Penzias and Robert Wilson weren’t looking for it, the hum that their antenna kept picking up turned out to be the afterglow radiation of the big bang. Today, it’s what we call the cosmic microwave background, and it’s critical to our understanding of the early universe.

  • Nothing — the antenna was faulty

Question 10 of 10

Astrophysicists like Katie Mack have theorized about potential endings to our universe! One of them is aptly named “heat death.” But what does that mean?

  • As the universe expands, everything will get farther and more isolated. Eventually, galaxies will be lonely, dark and cold.

    It might be trillions of years in the future, but the heat death ending of the universe is based on what we’ve observed about dark energy in the present. In this hypothetical ending, eventually galaxies would be so spread out and far away that the light from one could never reach the other. That’s one long-distance relationship!

  • The sun will gradually grow larger and larger until it becomes a supernova, engulfing Earth in a wave of heat.
  • Our galaxies will eventually collide and collapse, creating an ultramassive black hole that absorbs the rest of the universe into itself.
  • As space-time expansion accelerates, the friction of galaxies will “heat up” our universe until eventually every star system will become too hot to support life.

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