Solar system; stability of orbital motions; satellites key terms

space-63-term-01 classification Our Solar System

A classification cue for nebula cloud forming a protostar: it supports (Physics only) State that the Sun is a star by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-63-term-02 evidence Our Solar System

A evidence cue for main sequence star balancing forces: it supports (Physics only) State that the Sun is a star by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-65-term-01 classification Our Solar System

A classification cue for distant galaxy spectrum: it supports (Physics only) State that the Sun is one of many stars in the Milky Way galaxy by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: identify classify category label definition object type membership distinction.

space-65-term-02 evidence Our Solar System

A evidence cue for red-shifted absorption lines: it supports (Physics only) State that the Sun is one of many stars in the Milky Way galaxy by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-62-term-01 classification Our Solar System

A classification cue for distant galaxy spectrum: it supports (Physics only) State that the Milky Way galaxy is one of many billions of galaxies in the universe by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: identify classify category label definition object type membership distinction.

space-62-term-02 evidence Our Solar System

A evidence cue for red-shifted absorption lines: it supports (Physics only) State that the Milky Way galaxy is one of many billions of galaxies in the universe by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-25-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) Describe the Solar System as the Sun, planets, dwarf planets, moons, asteroids and comets by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-25-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) Describe the Solar System as the Sun, planets, dwarf planets, moons, asteroids and comets by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-60-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) State that planets and dwarf planets orbit the Sun by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-60-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) State that planets and dwarf planets orbit the Sun by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-58-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) State that moons orbit planets by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-58-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) State that moons orbit planets by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-09-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) Describe a moon as a natural satellite by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-09-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) Describe a moon as a natural satellite by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-11-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) Describe artificial satellites as human-made objects that orbit planets or moons by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-11-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) Describe artificial satellites as human-made objects that orbit planets or moons by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-30-term-01 classification Our Solar System

A classification cue for planet orbiting the Sun: it supports (Physics only) Distinguish planets from moons by what they orbit by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-30-term-02 evidence Our Solar System

A evidence cue for moon orbiting a planet: it supports (Physics only) Distinguish planets from moons by what they orbit by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-32-term-01 classification Our Solar System

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Distinguish stars from planets by explaining that stars produce their own light by fusion whereas planets do not by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-32-term-02 evidence Our Solar System

A evidence cue for main sequence star balancing forces: it supports (Physics only) Distinguish stars from planets by explaining that stars produce their own light by fusion whereas planets do not by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-26-term-01 classification Our Solar System

A classification cue for distant galaxy spectrum: it supports (Physics only) Distinguish a galaxy from the universe by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: identify classify category label definition object type membership distinction.

space-26-term-02 evidence Our Solar System

A evidence cue for red-shifted absorption lines: it supports (Physics only) Distinguish a galaxy from the universe by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-06-term-01 classification Our Solar System

A classification cue for Solar System order model: it supports (Physics only) Apply WS 1.4 when interpreting diagrams or models of the Solar System by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Solar System answers must distinguish stars, planets, moons, asteroids, comets, natural satellites and artificial satellites by what they are and what they orbit. Cue words: identify classify category label definition object type membership distinction.

space-06-term-02 evidence Our Solar System

A evidence cue for planet compared with a star: it supports (Physics only) Apply WS 1.4 when interpreting diagrams or models of the Solar System by linking the correct Space Physics object, stage, motion or evidence to Our Solar System. Solar System answers must distinguish stars, planets, moons, asteroids, comets, natural satellites and artificial satellites by what they are and what they orbit. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-10-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe a star as forming from a cloud of dust and gas called a nebula by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-10-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe a star as forming from a cloud of dust and gas called a nebula by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-20-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how gravitational attraction pulls dust and gas together to form a protostar by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-20-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how gravitational attraction pulls dust and gas together to form a protostar by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-66-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) State that the temperature rises as the protostar becomes denser by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-66-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) State that the temperature rises as the protostar becomes denser by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-49-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) State that a star enters the main sequence when it becomes hot enough for hydrogen nuclei to fuse to form helium by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-49-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) State that a star enters the main sequence when it becomes hot enough for hydrogen nuclei to fuse to form helium by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-39-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Explain that fusion of hydrogen nuclei releases energy in a main sequence star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-39-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Explain that fusion of hydrogen nuclei releases energy in a main sequence star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-36-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Explain that a main sequence star is stable because the forces within it are balanced by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-36-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Explain that a main sequence star is stable because the forces within it are balanced by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-22-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe the balance in a main sequence star as gravity acting inwards and pressure from fusion energy acting outwards by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-22-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe the balance in a main sequence star as gravity acting inwards and pressure from fusion energy acting outwards by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-64-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) State that the Sun is currently a main sequence star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-64-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) State that the Sun is currently a main sequence star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-15-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a star about the same size as the Sun becomes a red giant by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-15-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a star about the same size as the Sun becomes a red giant by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-13-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a red giant becomes a white dwarf by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-13-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a red giant becomes a white dwarf by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-19-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a white dwarf cools to become a black dwarf by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-19-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a white dwarf cools to become a black dwarf by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-16-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a star much more massive than the Sun becomes a red super giant by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-16-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a star much more massive than the Sun becomes a red super giant by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-14-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a red super giant may explode as a supernova by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-14-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a red super giant may explode as a supernova by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-50-term-01 classification The life cycle of a star

A classification cue for distant galaxy spectrum: it supports (Physics only) State that a supernova explosion distributes elements throughout the universe by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: identify classify category label definition object type membership distinction.

space-50-term-02 evidence The life cycle of a star

A evidence cue for red-shifted absorption lines: it supports (Physics only) State that a supernova explosion distributes elements throughout the universe by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Red shift means light from distant galaxies has increased wavelength; together with cosmic microwave background radiation it supports an expanding universe from the Big Bang. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-18-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a supernova can leave behind a neutron star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-18-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a supernova can leave behind a neutron star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-17-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Describe how a supernova can leave behind a black hole if the remaining mass is large enough by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-17-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Describe how a supernova can leave behind a black hole if the remaining mass is large enough by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-08-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Compare the life cycle of a Sun-sized star with the life cycle of a much more massive star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-08-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Compare the life cycle of a Sun-sized star with the life cycle of a much more massive star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-04-term-01 classification The life cycle of a star

A classification cue for nebula cloud forming a protostar: it supports (Physics only) Apply WS 1.2 when using models to represent stages in the life cycle of a star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: identify classify category label definition object type membership distinction.

space-04-term-02 evidence The life cycle of a star

A evidence cue for main sequence star balancing forces: it supports (Physics only) Apply WS 1.2 when using models to represent stages in the life cycle of a star by linking the correct Space Physics object, stage, motion or evidence to The life cycle of a star. Star life cycles depend on mass: nebula and protostar stages lead to main sequence, then lower-mass and higher-mass stars follow different final pathways. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-56-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) State that gravity provides the force that allows planets and satellites to maintain circular orbits by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-56-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) State that gravity provides the force that allows planets and satellites to maintain circular orbits by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-37-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Explain that an object moving in a circular orbit is accelerating because its velocity is changing direction by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-37-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Explain that an object moving in a circular orbit is accelerating because its velocity is changing direction by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-54-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) State that for a stable circular orbit the speed of the object is constant but its velocity changes by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-54-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) State that for a stable circular orbit the speed of the object is constant but its velocity changes by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-42-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Explain that the direction of the velocity of an orbiting object is at right angles to the force of gravity by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-42-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Explain that the direction of the velocity of an orbiting object is at right angles to the force of gravity by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-24-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Describe the force of gravity on an orbiting object as acting towards the centre of the orbit by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-24-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Describe the force of gravity on an orbiting object as acting towards the centre of the orbit by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-35-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Explain that a change in orbital radius changes the speed of an orbiting object by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-35-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Explain that a change in orbital radius changes the speed of an orbiting object by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-53-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) State that for a given central object, a smaller orbital radius is associated with a higher orbital speed by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-53-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) State that for a given central object, a smaller orbital radius is associated with a higher orbital speed by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-51-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) State that artificial satellites can orbit the Earth by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-51-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) State that artificial satellites can orbit the Earth by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-59-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) State that natural satellites such as moons can orbit planets by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-59-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) State that natural satellites such as moons can orbit planets by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-29-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Distinguish orbital motion from rotation by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-29-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Distinguish orbital motion from rotation by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-28-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Distinguish natural satellites from artificial satellites by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-28-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Distinguish natural satellites from artificial satellites by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-05-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Apply WS 1.4 when interpreting diagrams of orbital motion by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-05-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Apply WS 1.4 when interpreting diagrams of orbital motion by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.

space-01-term-01 classification Orbital motion, natural and artificial satellites

A classification cue for planet orbiting the Sun: it supports (Physics only) Apply MS 1c and MS 3b when interpreting proportional relationships between orbital radius and orbital speed by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: identify classify category label definition object type membership distinction.

space-01-term-02 evidence Orbital motion, natural and artificial satellites

A evidence cue for moon orbiting a planet: it supports (Physics only) Apply MS 1c and MS 3b when interpreting proportional relationships between orbital radius and orbital speed by linking the correct Space Physics object, stage, motion or evidence to Orbital motion, natural and artificial satellites. In orbital motion, gravity supplies the centripetal force, so the object keeps changing direction while remaining in a stable path around the body it orbits. Cue words: observation spectrum signal data measurement inference support pattern conclusion.