ESS 1-2 Seasons: Develop and use a model of the Earth-sun system to explain cyclical patterns of seasons, which includes the earth’s tilt and directional angle of sunlight on different areas of the Earth across the year.
I Cans: identify the parts of the Earth-Moon-Sun system, including axial tilt and the size and distance relationships of the model.
explain the causes of the seasons at given locations on Earth.
use a model to predict moon phases, eclipses, and seasons.
ESS 1-1 Lunar Phases and Eclipses: Develop and use a model of the Earth-sun-moon system to describe the cyclic patterns of lunar phases and eclipses of the sun and moon.
I Cans: identify the parts of the Earth-Moon-Sun system, including axial tilt and the size and distance relationships of the model.
describe the relationship between the orbit and rotations of the Earth and Moon.
describe the effects of solar energy on the Earth-Moon system.
explain moon phases when given the relative location of Earth, sun, and moon.
explain the processes that create solar and lunar eclipses, including the way sunlight is blocked for each type of eclipse.
use a model to predict moon phases and eclipses.
ESS1.B (ESS 1-4) Objects in The Solar System
Analyze and interpret data to determine scale properties of objects in the solar system.
I Cans: organize data about solar system objects.
describe patterns in the data by comparing and contrasting solar system objects (planets, moons, asteroids, meteors, & comets)
identify advances in space science and connections to everyday uses
use data patterns to draw conclusions about characteristics of solar system objects (features, composition, and locations)
use data patterns to illustrate scale differences in solar system objects
draw conclusions about patterns in data that show the existence of unobservable phenomena (Objects too big or too small to directly observe)
ESS 1-3 Universe: Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.
I Cans: identify the components of the universe, including galaxies and solar systems (sun, planets, moons, asteroids).
identify the role of gravity in the universe.
describe the impact of mass of objects and distance between them on gravity.
describe the orbital motion of objects in the universe and the pattern of gravitational forces that create this motion.
explain the formation of bodies in the universe, as it was driven by gravitational forces.
I Cans: identify the parts of the Earth-Moon-Sun system, including axial tilt and the size and distance relationships of the model.
explain the causes of the seasons at given locations on Earth.
use a model to predict moon phases, eclipses, and seasons.
ESS 1-1 Lunar Phases and Eclipses: Develop and use a model of the Earth-sun-moon system to describe the cyclic patterns of lunar phases and eclipses of the sun and moon.
I Cans: identify the parts of the Earth-Moon-Sun system, including axial tilt and the size and distance relationships of the model.
describe the relationship between the orbit and rotations of the Earth and Moon.
describe the effects of solar energy on the Earth-Moon system.
explain moon phases when given the relative location of Earth, sun, and moon.
explain the processes that create solar and lunar eclipses, including the way sunlight is blocked for each type of eclipse.
use a model to predict moon phases and eclipses.
ESS1.B (ESS 1-4) Objects in The Solar System
Analyze and interpret data to determine scale properties of objects in the solar system.
I Cans: organize data about solar system objects.
describe patterns in the data by comparing and contrasting solar system objects (planets, moons, asteroids, meteors, & comets)
identify advances in space science and connections to everyday uses
use data patterns to draw conclusions about characteristics of solar system objects (features, composition, and locations)
use data patterns to illustrate scale differences in solar system objects
draw conclusions about patterns in data that show the existence of unobservable phenomena (Objects too big or too small to directly observe)
ESS 1-3 Universe: Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.
I Cans: identify the components of the universe, including galaxies and solar systems (sun, planets, moons, asteroids).
identify the role of gravity in the universe.
describe the impact of mass of objects and distance between them on gravity.
describe the orbital motion of objects in the universe and the pattern of gravitational forces that create this motion.
explain the formation of bodies in the universe, as it was driven by gravitational forces.