- Velocity (v) = Displacement (Δx) / Time (Δt): This tells you how fast something is moving and in what direction. Remember, velocity is not just speed; it's speed with direction.
- Acceleration (a) = Change in Velocity (Δv) / Time (Δt): Acceleration describes how quickly the velocity changes. A positive acceleration means you're speeding up, while a negative one means you're slowing down.
- v = u + at: This links final velocity, initial velocity, acceleration, and time.
- s = ut + (1/2)at²: This connects displacement, initial velocity, time, and acceleration.
- v² = u² + 2as: This relates final velocity, initial velocity, acceleration, and displacement, without needing to know the time.
- s = (1/2)(u + v)t: This ties together displacement, initial velocity, final velocity, and time.
- s = vt - (1/2)at²: This is similar to equation 2, but uses the final velocity instead of the initial velocity.
- Newton's First Law (Law of Inertia): An object at rest stays at rest, and an object in motion stays in motion with the same speed and in the same direction unless acted upon by a force.
- Newton's Second Law: F = ma: This is arguably the most important equation in mechanics. It states that the net force acting on an object is equal to its mass times its acceleration. Understanding this relationship is crucial for solving force-related problems.
- Newton's Third Law: For every action, there is an equal and opposite reaction. When you push on something, it pushes back on you with the same force.
- Work (W) = Fdcosθ: Work is done when a force causes a displacement. The angle θ is between the force and the displacement vectors.
- Kinetic Energy (KE) = (1/2)mv²: This is the energy an object possesses due to its motion.
- Potential Energy (PE) = mgh: This is the energy an object possesses due to its height above a reference point (usually the ground).
- Power (P) = W/t: Power is the rate at which work is done.
- Momentum (p) = mv: Momentum is a measure of an object's mass in motion.
- Impulse (J) = FΔt = Δp: Impulse is the change in momentum of an object.
- Coulomb's Law: F = k(q1q2/r²): This law describes the force between two point charges. The force is directly proportional to the product of the charges and inversely proportional to the square of the distance between them. Remember that like charges repel and opposite charges attract.
- Electric Field (E) = F/q: The electric field is the force per unit charge at a given point in space.
- Electric Potential (V) = k(q/r): Electric potential is the potential energy per unit charge at a given point in space. It's a scalar quantity, unlike the electric field, which is a vector.
- Ohm's Law: V = IR: This is a cornerstone of circuit analysis. It states that the voltage across a resistor is equal to the current through it times its resistance.
- Power (P) = IV = I²R = V²/R: Power in a circuit is the rate at which electrical energy is converted into other forms of energy (like heat or light).
- Resistors in Series: Req = R1 + R2 + R3 + ...: When resistors are connected in series, their equivalent resistance is the sum of their individual resistances.
- Resistors in Parallel: 1/Req = 1/R1 + 1/R2 + 1/R3 + ...: When resistors are connected in parallel, their equivalent resistance is calculated using this reciprocal formula.
- Magnetic Force on a Moving Charge: F = qvBsinθ: This is the force on a charge moving in a magnetic field. The force is proportional to the charge, the velocity, the magnetic field strength, and the sine of the angle between the velocity and the magnetic field vectors.
- Magnetic Force on a Current-Carrying Wire: F = ILBsinθ: This is the force on a wire carrying a current in a magnetic field. The force is proportional to the current, the length of the wire, the magnetic field strength, and the sine of the angle between the wire and the magnetic field vectors.
- Faraday's Law: ε = -N(ΔΦ/Δt): This law states that the induced electromotive force (EMF) in a circuit is equal to the negative of the number of turns in the coil times the rate of change of magnetic flux through the coil. This is the principle behind generators and transformers.
- Wave Speed (v) = fλ: This relates the speed of a wave to its frequency (f) and wavelength (λ).
- Period (T) = 1/f: The period is the time it takes for one complete cycle of the wave.
- Snell's Law: n1sinθ1 = n2sinθ2: This law describes how light bends when it passes from one medium to another. The indices of refraction (n1 and n2) are measures of how much the speed of light is reduced in each medium.
- Index of Refraction (n) = c/v: The index of refraction is the ratio of the speed of light in a vacuum (c) to the speed of light in the medium (v).
- Thin Lens Equation: 1/f = 1/do + 1/di: This equation relates the focal length (f) of a lens to the object distance (do) and the image distance (di).
- Magnification (M) = -di/do: Magnification describes how much larger or smaller the image is compared to the object. A negative magnification indicates an inverted image.
- Double-Slit Interference: dsinθ = mλ: This equation gives the angles at which constructive interference occurs in a double-slit experiment. The integer m is the order of the interference maximum.
- Single-Slit Diffraction: wsinθ = mλ: This equation gives the angles at which destructive interference (minima) occurs in single-slit diffraction. Here, w is the width of the slit.
- First Law of Thermodynamics: ΔU = Q - W: This is the law of conservation of energy for thermodynamic systems. The change in internal energy (ΔU) of a system is equal to the heat added to the system (Q) minus the work done by the system (W).
- Ideal Gas Law: PV = nRT: This law relates the pressure (P), volume (V), number of moles (n), ideal gas constant (R), and temperature (T) of an ideal gas.
- Work Done by a Gas at Constant Pressure: W = PΔV: This formula gives the work done when a gas expands or compresses at constant pressure.
- Heat Transfer (Q) = mcΔT: This equation calculates the heat required to change the temperature of a substance. The specific heat capacity (c) is a property of the substance.
- Change in Entropy (ΔS) = Q/T: Entropy is a measure of the disorder or randomness of a system. The change in entropy is equal to the heat transferred reversibly divided by the temperature.
Hey guys! Physics in high school can feel like navigating a maze filled with abstract concepts and, of course, formulas. But don't worry; having a solid formula sheet can be a lifesaver. Think of it as your trusty map through the physics landscape. In this article, we're going to break down the essential formulas you'll likely encounter, making them easier to understand and apply. Buckle up, and let's dive in!
Mechanics Formulas
When it comes to mechanics formulas, this is where you'll spend a significant amount of your time, as these formulas are used to calculate the motion of objects and the forces acting on them. Understanding these principles is super crucial for grasping more advanced topics later on. Let's start with kinematics, which is all about describing motion without worrying about what causes it. You've got your basic equations like:
Then, you get into the uniformly accelerated motion equations, often referred to as the 'Big Five' or SUVAT equations (where SUVAT stands for Displacement (s), Initial Velocity (u), Final Velocity (v), Acceleration (a), and Time (t)). These are your go-to tools for solving most kinematic problems:
These equations are powerful, but remember they only work when the acceleration is constant and in a straight line! Be careful to choose the right equation based on the information you have and what you're trying to find. Next up, dynamics, which brings forces into the mix. Newton's Laws of Motion are the bedrock here:
Other important concepts include work, energy, and power:
Finally, momentum and impulse:
Understanding these mechanics formulas is fundamental to tackling a wide range of physics problems. Make sure you practice using them in different scenarios to build your confidence!
Electricity and Magnetism Formulas
Alright, let's switch gears and delve into the world of electricity and magnetism formulas. This is where things get really interesting, especially when you start seeing how these two phenomena are intertwined. First off, let's cover the basics of electrostatics:
Next up are circuit elements and circuit analysis:
Now, let's move on to magnetism:
Finally, let's touch on electromagnetic induction:
These formulas are essential for understanding how electricity and magnetism work, both separately and together. Practice applying them in various scenarios to really solidify your understanding.
Waves and Optics Formulas
Now let's explore waves and optics formulas! Waves are disturbances that transfer energy through a medium, and optics is the study of light and its behavior. Understanding these concepts is crucial for understanding phenomena like sound, light, and even quantum mechanics later on. First, let's look at some basic wave properties:
Next, we'll examine some formulas related to optics, focusing mainly on geometrical optics:
Then, we can explore some interference and diffraction formulas:
Understanding these wave and optics formulas will help you to explain many common phenomena, from the colors of a rainbow to how lenses work in cameras and telescopes. Practice is essential for getting comfortable with these equations.
Thermodynamics Formulas
Let's switch gears one more time and explore thermodynamics formulas. Thermodynamics deals with heat, work, and energy transfer. These formulas are used to describe how energy flows in physical systems and how it relates to temperature and entropy.
Then we can explore heat transfer:
Lastly, entropy and the second law of thermodynamics:
Understanding these thermodynamics formulas will allow you to analyze and predict the behavior of systems involving heat transfer and energy conversion. These principles are vital in fields ranging from engineering to chemistry.
So, there you have it – a rundown of the essential physics formulas you'll likely encounter in high school. Remember, physics isn't just about memorizing formulas; it's about understanding the concepts behind them. Keep practicing, keep asking questions, and you'll be mastering physics in no time! Good luck, and have fun with it!
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