Docsity
Docsity

Prepare for your exams
Prepare for your exams

Study with the several resources on Docsity


Earn points to download
Earn points to download

Earn points by helping other students or get them with a premium plan


Guidelines and tips
Guidelines and tips

Astronomy Equation Cheat Sheet for the 1st Midterm, Cheat Sheet of Astronomy

Here you have the essential Astronomy equations

Typology: Cheat Sheet

2019/2020

Uploaded on 11/27/2020

ekaatma
ekaatma 🇺🇸

4.2

(34)

268 documents

1 / 5

Toggle sidebar

This page cannot be seen from the preview

Don't miss anything!

bg1
EQUATION SHEET - FIRST MID-TERM
Astronomy 103, Fall 2007
Prof. Alex Lazarian, TA Katie Devine
The following equations come from your homework, with a few extras thrown in for good
measure. When in doubt about how to use an equation or what it means, consult your
book for more information!
ALWAYS CHECK UNITS TO MAKE SURE YOUR ANSWERS MAKE SENSE!
1. Circumference of a Circle:
C= 2πR
C is Circumference
R is the Radius of the circle
2. Angular size vs. Real Size
Ao
360o=L
C
or
L=dA
57.3o
A is the number of degrees (the Angle) an object covers on the sky
L is the real size of the object
C is the circumference of the circle on the celestial sphere at distance d
d is the distance to the object
3. Kepler’s Third Law
P2=A3
P is orbital period in Years
pf3
pf4
pf5

Partial preview of the text

Download Astronomy Equation Cheat Sheet for the 1st Midterm and more Cheat Sheet Astronomy in PDF only on Docsity!

EQUATION SHEET - FIRST MID-TERM

Astronomy 103, Fall 2007

Prof. Alex Lazarian, TA Katie Devine

The following equations come from your homework, with a few extras thrown in for good measure. When in doubt about how to use an equation or what it means, consult your book for more information!

ALWAYS CHECK UNITS TO MAKE SURE YOUR ANSWERS MAKE SENSE!

  1. Circumference of a Circle:

C = 2πR

C is Circumference R is the Radius of the circle

  1. Angular size vs. Real Size

360 Aoo^ =^ CL

or

L = d ∗ 57 A. 3 o

A is the number of degrees (the Angle) an object covers on the sky L is the real size of the object C is the circumference of the circle on the celestial sphere at distance d d is the distance to the object

  1. Kepler’s Third Law

P 2 = A^3

P is orbital period in Years

A is orbital distance (semimajor axis) in AU

Modified Kepler’s Third Law:

MA + MB = PA 32 ((AUY R^ ))

MA and MB are the masses of two bodies orbiting each other P is orbital period in Years A is orbital distance between the two bodies in AU

  1. Force and Acceleration

F = Ma

F is force M is the mass of the object acted on by the force a is the acceleration the mass gets from the force

a = V T^11 −−VT^22 a is the acceleration

V 1 is the initial velocity V 2 is the final velocity T 1 is the initial time T 2 is the final time so, V 1 − V 2 is the change in velocity and T 1 − T 2 is the change in time

  1. Force from gravity (Universal Law of Gravity)

Fgravity = mM G d 2

Fgravity is Force of gravity between two objects m is the mass of one of the objects M is the mass of the other object

V =

√GM

R V is orbital velocity G is gravitational constant M is mass of object being orbited R is the radius of the orbit

  1. Escape Velocity

Vesc =

2 GM R V is escape velocity G is gravitational constant M is mass of object being escaped R is the radius of the planet/object being escaped

  1. Energy

EK = 12 mV 2

EK is the Kinetic Energy of an object m is mass of the object V is the velocity of the object

EP = −GmM d

EP is the Potential Energy of an object m is the mass of the object with gravitational potential energy M is mass of the object giving gravitation potential energy G is gravitational constant d is distance between center of mass m and mass M

  1. Angular Momentum

L = mvr

L is the angular momentum of an object in a circular orbit m is the mass of the object r is the radius of the orbit