Physics · Professor Newton

Space and gravity, Year 9:全部卡片

整套按顺序列出——孩子看到之前,您可以先通读一遍。

1 KS3-PHYS-SPA-0013

On Mars, the gravitational field strength g is about 4 N/kg. What is the weight of a 50 kg astronaut on Mars?

200 N

提示Every kilogram of her is pulled down with the force given for that planet.

为什么Weight = mass × g, so 50 × 4. On Earth, where g is 10 N/kg, the same astronaut weighs 500 N. She is the same person with the same mass; only the pull on each kilogram has changed.

2 KS3-PHYS-SPA-0014

An astronaut has a mass of 80 kg on Earth. What is her mass on the Moon?

80 kg

提示Ask whether the journey has added or removed any of the matter she is made of.

为什么Mass is the amount of matter in an object, and travelling does not change it. What changes on the Moon is her weight, the force of gravity on that mass, which is about a sixth of its value on Earth.

3 KS3-PHYS-SPA-0015

A space probe weighs 200 N on Earth, where g is 10 N/kg. What would it weigh close to Jupiter, where g is about 25 N/kg?

500 N

提示Find the one thing about the probe that stays fixed wherever it goes, then use the new planet's pull.

为什么First find the mass: 200 ÷ 10 = 20 kg. That mass is the same at Jupiter, so the weight there is 20 × 25. Going by way of the mass is the safe route between any two worlds.

4 KS3-PHYS-SPA-0016

An astronaut can jump much higher on the Moon than on Earth, although her muscles are no stronger there. Why?

The Moon pulls her down with a smaller force

提示Her legs push just as hard as at home, so ask what is working against them.

为什么The Moon's gravitational field strength is about a sixth of the Earth's, so her weight is about a sixth of what it was. The same push from her legs is opposed by a much weaker downward force, and she rises further before it brings her back.

5 KS3-PHYS-SPA-0017

Stars shine with light of their own. Where does the light we see from a planet such as Venus come from?

It is sunlight reflected off the planet

提示Venus makes none itself, so think about what is shining on it.

为什么Planets are not hot enough to glow visibly. We see them the same way we see the Moon: light from our star falls on them and some bounces back towards us. That is one way to tell a planet from a star, however alike they look to the eye.

6 KS3-PHYS-SPA-0018

A huge ball of hot, glowing gas that gives out its own light

A star

提示Our solar system has exactly one, at its centre.

为什么The Sun is one of these seen from close by, and every point of light in a constellation is another seen from very far away. Many of them are bigger and brighter than the Sun; distance alone makes them look like pinpricks.

7 KS3-PHYS-SPA-0019

The nearest star to the Earth is the ____.

Sun

提示You can see it without waiting for night.

为什么It is easy to forget that the bright disc in the daytime sky belongs in the same family as the points of light at night. The next nearest is so much further away that its light takes over four years to arrive.

8 KS3-PHYS-SPA-0020

The Earth is one planet in the solar system. The solar system is one tiny part of a ____, and billions of these together make up the ____.

galaxy; universe

提示Each step up contains everything that came before it.

为什么The Earth is one planet among several around the Sun. The Sun is one star among billions in the Milky Way. The Milky Way is one among billions of similar collections. Each step is a vast jump in size.

9 KS3-PHYS-SPA-0021

An enormous system of stars, gas and dust held together by gravity

A galaxy

提示Andromeda is a famous one, and we live inside another.

为什么Stars are not scattered evenly through space. They are gathered into these great systems, with almost empty space in between. Seen from far outside, a whole one looks like a single faint smudge of light.

10 KS3-PHYS-SPA-0022

The galaxy that contains our Sun

The Milky Way

提示On a very dark night it shows as a pale, cloudy band right across the sky.

为什么It is a flat spiral, and the Sun sits out in one of its arms, roughly halfway from the centre to the edge. The band we see at night is our own galaxy viewed edge-on from the inside.

11 KS3-PHYS-SPA-0023

Roughly how many stars does a galaxy like ours contain: thousands, millions or billions?

Billions

提示Far more than there are people on Earth.

为什么Estimates for our own galaxy run to at least a hundred thousand million stars. Only a few thousand are bright enough and near enough to see without a telescope, so the night sky shows a tiny sample.

12 KS3-PHYS-SPA-0024

A star is 50 light years from the Earth. If it exploded today, in how many years would people on Earth first see the explosion? (number only)

50

提示The news can only reach us by travelling here as light.

为什么A light year is the distance light covers in one year, so light from something 50 of them away takes 50 years to make the trip. Until that light arrives, the star would look exactly as it always has.

13 KS3-PHYS-SPA-0025

Why is looking at a very distant galaxy like looking into the past?

Its light set off long ago

提示Think about how old the picture is by the time it reaches your telescope.

为什么We never see a distant object as it is now, only as it was when the light we are receiving left it. For a galaxy millions of light years away, that light began its journey millions of years ago.

14 KS3-PHYS-SPA-0026

Why do astronomers give the distances to stars in light years rather than in kilometres?

In kilometres the numbers would be unmanageably huge

提示Try writing the distance to the next star using a unit made for road journeys.

为什么One light year is about 9.5 million million kilometres, and even the nearest star beyond the Sun is more than four of them away. A unit sized for the job keeps the numbers small enough to read and compare.

15 KS3-PHYS-SPA-0027

Light from the nearest star beyond the Sun takes about ____ years to reach us.

4

提示More than the 8 minutes sunlight takes, but fewer than ten years.

为什么That star is a little over four light years away. Light from the Sun arrives in about eight minutes, which shows how much emptier the space between stars is than the space inside our solar system.

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