1. Arrange students into groups. Each group needs at least ONE person who has a mobile device.
2. If their phone camera doesn't automatically detect and decode QR codes, ask students to
4. Cut them out and place them around your class / school.
1. Give each group a clipboard and a piece of paper so they can write down the decoded questions and their answers to them.
2. Explain to the students that the codes are hidden around the school. Each team will get ONE point for each question they correctly decode and copy down onto their sheet, and a further TWO points if they can then provide the correct answer and write this down underneath the question.
3. Away they go! The winner is the first team to return with the most correct answers in the time available. This could be within a lesson, or during a lunchbreak, or even over several days!
4. A detailed case study in how to set up a successful QR Scavenger Hunt using this tool can be found here.
Question | Answer |
1. Point in which the planet’s orbit is farthest from the sun | Aphelion | 2. The distance from the center of the Earth to the center of the Sun | Astronomical Unit | 3. Defines the shape for a planets elliptical orbit | Eccentricity | 4. Point in a planets orbit when it is closest to the sun | Perihelion | 5. Planets backwards motion in the sky | Retrograde Motion | 6. Jupiter, Saturn, Uranus and Neptune are examples of | Gas Giant Planets | 7. The wobble in Earths rotational Axis | Procession | 8. Rocky-surfaced planets are examples of | Terrestrial Planets | 9. The wing going in different directions on Saturn | Belt | 10. Material that makes up Saturn and Jupiter (non-earthly substance) | Liquid Metallic Hydrogen | 11. The light colored stripes of Jupiter are called | Zone | 12. A variable star that pulsates both temperature and brightness | Cepheid Variable | 13. A type of ring of stars that surround most disk galaxies | Halo | 14. A very bright variable star (found in globular clusters) | RR Lyrae Variable | 15. The raveling up of a galaxy | Spiral Density Waves | 16. A type of star that brightness changes, regularly or irregularly | Variable Star | 17. compact region at the center of a galaxy that has a much higher than normal luminosity over at least some portion of the electromagnetic spectrum | Active Galactic Nucleus | 18. Unit that explains the constant rate of how the universe is expanding | Hubble Constant | 19. Extremely active galactic nucleus, emits large amounts of energy. Supposedly has many massive Black Holes near the center | Quasar | 20. Galaxy;emits radiation in the radio frequency on the electromagnetic spectrum | Radio Galaxy | 21. large group of smaller galaxy cluster or galaxy groups | super cluster | 22. Celestial body that could or did come together from gravitation of planets | Planetesimal | 23. Solid central part of a comet | Nucleus | 24. Theory of which the universe started from nothing, and we came from a big explosion | Big Bang Theory | 25. Radiation from the early stages of the universe(or the Big Bang) | Cosmic Background Radiation | 26. Study of the origin and development of the universe | cosmology | 27. The exponentially fast expansion of the universe after the Big Bang | Inflationary Universe | 28. The theory that there is no end to the universe | Steady State Theory | 29. A small rocky body that is orbiting the sun or other celestial bodies | Asteroid | 30. Nebulous envelope around the nucleus of a comet | Coma | 31. Small icy celestial body made of ice, carbon dioxide etc | Comet | 32. Small rocky or metallic body in outer space that enters Earth atmosphere(Smaller then asteroids) | Meteor | 33. Celestial event when tons of meteors seem to radiate, or originate from one point in the sky | Meteor Shower | 34. The term for a meteor that passes through Earth's atmosphere and touches the surface | Meteorite | 35. Small rocky or metallic body in outer space that doesn't enter Earths atmosphere | Meteoroid | 36. All existing matter and space as a whole;or cosmos | Universe | 37. A group of millions and billions of stars held together by gravitational pulls | Galaxy | 38. The scientific theory that planets orbit in a elliptical orbit | Kepler's 1st Law | 39. The scientific theory that as a planet nears the sun it gets faster and as it gets further away it slows down | Kepler's Second Law | 40. The theory that if you square the 'year' of each planet, and divide it by the cube of its distance to the Sun, you get the same number, for all planets. | Kepler's 3rd Law | 41. The wobble in Earths rotational Axis | Procession | 42. periodic variation in the inclination of the axis of a rotating object | Nutation | 43. he center of mass of two or more bodies that orbit one another and is the point about which the bodies orbit | Barycenter |
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