Standards IE d,,k Students will recognize the usefulness and limitations of models and theories. Students will formulate explanations using logic and evidence Objectiv e 1 Describe 2 lines of evidence for Earth’s rotation Objectiv e 2 Explain how constellations show evidence for Earth’s rotation Objectiv e 3 Explain Earth’s seasons Assessme Chapter Test Chapter 26, Section 2
11
Embed
Standards IE d,,k Students will recognize the usefulness and limitations of models and theories. Students will formulate explanations using logic and evidence.
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
Standards IE d,,k Students will recognize the usefulness and limitations of models and theories. Students will formulate explanations using logic and evidence
Objective 1 Describe 2 lines of evidence for Earth’s rotation
Objective 2 Explain how constellations show evidence for Earth’s rotation
Objective 3 Explain Earth’s seasons
Assessment Chapter Test
Review Daily Bellwork, Science Starters, Standards Practice
Chapter 26, Section 2
Vocabulary
• Create flashcards and study the following words:– Rotation– Revolution– Perihelion– Aphelion– Equinox– Solstice
The Rotating Earth
• The spinning of the Earth on its Axis is called ROTATION.
• Rotation creates Day and Night• Evidence of Rotation—– Foucault Pendulum– Coriolis Effect– Day and Night
The Revolving Earth
• Earth spins on its axis (rotation) and it also travels or REVOLVES around the sun
• Complete revolution of the sun takes 365 ¼ days.
• Every four years we add a day…leap year• Perihelion=point in orbit closest to the sun• Aphelion =point in orbit farthest from the sun
Evidence of Earth’s Motion
Evidence of Rotation• If you watch the night sky
over a couple of hours, the stars and constellation patterns appear to move in the sky
• The moon and sun also appear to change places in the sky
Evidence of Revolution• Over several weeks a
constellations place in the sky will appear to change and at different times of year, different constellations will be visible.
• See pictures page 669
Measuring Time
• Earth’s motion is the basis for measuring time• One day is 24 hours—the amount of time it
takes Earth to rotate (spin on its axis)• One year is 365 ¼ days –the amount of time it
takes to travel (revolve) around the sun
Calendar
• Ancient civilizations:– Egyptians first to use a solar year– Aztecs used a stone calendar to know when to
plant– Julius Caesar began leap year
• Modern Calendar:– 1500s, Pope Gregory XIII created a calendar to fit
the seasons
AztecMayan
ROMAN
Measuring Time
• Time Zones—24 1 hour periods
Seasons
• Fall and Spring begin on an EQUINOX• Winter and Summer begin on a SOLSTICE• Brain Pop—Seasons and Solstice and Equinox
Interactive/Assessment
• Constellation Project!
INTERACTIVE/Assessment
Use the diagram on page 562 or the one below and copy and label it in your notes.