Year 10 Science - Waves, Motion, and Reactions Flashcards

0.0(0)
Studied by 0 people
call kaiCall Kai
Locked
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/38

flashcard set

Earn XP

Description and Tags

Comprehensive vocabulary flashcards covering Year 10 Science topics: Waves (Properties, Sound, Light), Motion (Newton's Laws, Kinematics), and Chemical/Nuclear Reactions.

Last updated 3:08 AM on 8/4/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai
Chat

No analytics yet

Send a link to your students to track their progress

39 Terms

1
New cards

Mechanical waves

Waves that require a medium (solidsolid, liquidliquid, or gasgas) to travel through, such as sound, water, or seismic waves.

2
New cards

Electromagnetic (EM) waves

Waves that do not need a medium and can travel through a vacuum at the speed of light (3×108m/s3 \times 10^8\,m/s).

3
New cards

Transverse waves

Waves in which particles vibrate perpendicular (at right angles) to the direction of travel, such as light or water waves.

4
New cards

Longitudinal waves

Waves in which particles vibrate parallel (in the same direction) to the direction of travel, consisting of compressions and rarefactions.

5
New cards

Amplitude

The maximum displacement of a particle from its rest position, which relates to the energy, loudness, or brightness of a wave.

6
New cards

Wavelength (λ\lambda)

The distance between two successive identical points on a wave, such as crest to crest, measured in metres (mm).

7
New cards

Frequency (ff)

The number of complete wave cycles passing a fixed point per second, measured in Hertz (HzHz).

8
New cards

Period (TT)

The time taken for one complete wave cycle, calculated as T=1fT = \frac{1}{f}.

9
New cards

The wave equation

The mathematical relationship where speed equals frequency multiplied by wavelength (v=fλv = f\lambda).

10
New cards

Doppler effect

The apparent change in frequency or pitch of a wave caused by the relative motion between the source and the observer.

11
New cards

Cochlea

The part of the inner ear filled with fluid and hair cells that converts sound vibrations into electrical nerve signals.

12
New cards

Absorption

A light behavior where energy is taken in by a material and typically converted to heat.

13
New cards

Reflection

A light behavior where light bounces off a surface, following the law that the angle of incidence equals the angle of reflection.

14
New cards

Refraction

The bending of light as it passes from one medium to another of different density because its speed changes.

15
New cards

Scattering

The redirection of light rays in many different directions after striking small particles, which explains why the sky appears blue.

16
New cards

Displacement

A vector quantity representing the straight-line distance from a start point to an end point, including direction.

17
New cards

Velocity

A vector quantity defined as displacement divided by time (vav=ΔsΔtv_{av} = \frac{\Delta s}{\Delta t}).

18
New cards

Acceleration (aa)

The rate of change of velocity over time, measured in m/s2m/s^2, calculated as a=ΔvΔta = \frac{\Delta v}{\Delta t}.

19
New cards

Inertia

The resistance of an object to a change in its motion, which is the focus of Newton's First Law.

20
New cards

Newton's Second Law

The law stating that the acceleration of an object is directly proportional to the net force and inversely proportional to its mass (F=maF = ma).

21
New cards

Newton's Third Law

The law stating that for every action force, there is an equal and opposite reaction force.

22
New cards

Law of Conservation of Mass

The principle that mass is neither created nor destroyed in a chemical reaction; the total mass of reactants equals the total mass of products.

23
New cards

Closed system

An experimental setup where no matter can enter or exit, allowing for the accurate demonstration of mass conservation.

24
New cards

IUPAC naming

A systematic, internationally agreed method for naming chemical compounds, such as using prefixes for covalent compounds.

25
New cards

Synthesis reaction

A reaction where two or more simple substances combine to form one more complex product (A+BABA + B \rightarrow AB).

26
New cards

Decomposition reaction

A reaction where one compound breaks down into two or more simpler substances (ABA+BAB \rightarrow A + B).

27
New cards

Neutralisation

A chemical reaction where an acid and a base react to form a salt and water.

28
New cards

Precipitation reaction

A type of double displacement reaction where two aqueous ionic compounds react to form an insoluble solid.

29
New cards

Exothermic reaction

A reaction that releases energy (usually heat) to the surroundings, making the surroundings feel warmer.

30
New cards

Endothermic reaction

A reaction that absorbs energy from the surroundings, making the surroundings feel cooler.

31
New cards

pH scale

A measure of acidity or alkalinity ranging from 00 to 1414, where 77 is neutral.

32
New cards

Collision Theory

The theory that reactions occur when particles collide with sufficient energy (activation energy) and the correct orientation.

33
New cards

Activation energy

The minimum amount of energy that colliding particles need for a chemical reaction to occur.

34
New cards

Catalyst

A substance that increases the reaction rate by providing an alternative pathway with lower activation energy without being consumed.

35
New cards

Alpha (α\alpha) decay

Radioactive decay where a nucleus emits a particle of 22 protons and 22 neutrons, decreasing the mass number by 44 and atomic number by 22.

36
New cards

Beta (β\beta) decay

Radioactive decay where a neutron converts into a proton, emitting a fast-moving electron, increasing the atomic number by 11.

37
New cards

Half-life

The time taken for half of the radioactive atoms in a sample to undergo decay.

38
New cards

Nuclear fission

The process of splitting a large, unstable nucleus into smaller nuclei, releasing energy.

39
New cards

Nuclear fusion

The process where small nuclei combine to form a larger nucleus, releasing energy; this process powers the Sun.