Term 2 review: Earth’s resources and patterns in the sky
الأسبوع 30 · مراجعة الفصل الدراسي الثاني: الموارد الموجودة على سطح الأرض والأنماط في السماء · 3 دروس
3
Review: gravity, sky and stars
Discovery Education Science P5: Term 2, Units 3–4
GoalReview gravity, rotation and revolution, shadows, the Moon, constellations and star brightness with new questions.
New words
gravity · a pull between objects that have mass, stronger for more mass and for less distanceorbit · the curved path of one object around anotherapparent brightness · how bright a star looks from Earth
Explanation
Forces are pushes and pulls. Gravity is a pull between any two objects that have mass. Earth’s gravity pulls toward its centre, which is what “down” means, and it holds the Moon in orbit, while the Sun’s gravity holds the planets. Without air all objects would fall together, and air resistance slows paper and feathers. Earth rotates once in about a day, which makes day and night and makes the Sun and stars seem to rise in the east and set in the west. It revolves round the Sun in about a year. Earth’s axis keeps the same tilt, about 23½°, and points the same way, so as Earth goes round, different parts lean toward the Sun and we get seasons. Shadows are shortest around midday. The Moon shines by reflecting sunlight, and its phases come from how much of the lit half we see. The Sun is a star that looks brightest because it is the closest. Never look at the Sun.
Idea
Remember
rotation
about 24 hours; day and night
revolution
about a year; with the tilt, seasons
gravity
more mass, stronger; farther, weaker
star brightness
near looks bright, far looks dim
Worked examples
Earth turns 15° each hour. In 9 hours it turns 9 × 15 = 135°. A full turn is 360°, so there are 360 − 135 = 225° left to turn.
Day
Shadow (cm)
1
52
2
55
3
58
Three shadow lengths of a post are 52 cm, 55 cm and 58 cm on three different days at the same time. The average is (52 + 55 + 58) ÷ 3 = 165 ÷ 3 = 55 cm. Averaging makes a result more trustworthy.
A torch gives 600 units at 1 m and 150 units at 2 m. The brightness is 600 ÷ 150 = 4 times smaller when the distance is doubled. A star twice as far looks 4 times dimmer.
Class activity
Sky journal (a grown-up helps; never look at the Sun). For one week, write each evening whether you can see the Moon and draw its shape. Find the Pole Star with a grown-up and draw one constellation you can see. In the daytime measure the shadow of a pole at the same hour on three days. Write one thing that stayed the same and one that changed. Which Term 2 idea explains each?
Practice
1
Two balls of different mass are dropped together from knee height onto a mat. What do you expect, and why?
They land about together, because with little air resistance mass does not change how fast things fall.
2
Which Moon shape is hidden behind the ? in the row, the one with no lit part visible? Say its name.
The new Moon.
3
True or false: the Sun is the brightest star because it is the biggest. Give a reason.
False. It looks brightest because it is the closest. Other stars can be bigger.
4
A shadow is 180 cm at 9:00, 120 cm at 10:30 and 100 cm at noon. How much did it shorten from 9:00 to noon? When is it shortest?
Time
Shadow (cm)
9:00
180
10:30
120
noon
100
180 − 100 = 80 cm shorter. It is shortest around noon, when the Sun is highest.