celestial mechanics phys390 (astrophysics) professor lee carkner lecture 5
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Celestial Mechanics
PHYS390 (Astrophysics)
Professor Lee Carkner
Lecture 5
Questions
1) Can we achieve enormous resolving power by dramatically increasing N?
Answer: NoExplain: The more slits, the larger the grating has to be.
Large gratings require the light to be more spread out, need higher intensity.
2) Can we achieve enormous resolving power by using very high orders?
Answer: NoExplain: Increase n, decrease brightness, need higher
intensity to use higher orders.
Test #1
Next Wednesday, Dec 1 Multiple choice (25%)
Like in-class questions
Problems (75%) Like PALs and homework
Sample equation sheet on web page Just need pencil and calculator
Kepler’s Laws In the 1600’s Johannes Kepler
used Tycho Brahe’s data to find the laws of planetary motion
Kepler’s First Law
Half of the longest (major) axis is the semi-major axis called a
Half the distance between the foci is called c
e = c/a
e = 0 is circle (a=r) e = 1 is line
c a
Kepler’s Third Law
There is a relationship between the orbital size and period
Only in the solar system
and if P is in years and a is in AU
P2=[42/G(m1+m2)] a3
Where m1 and m2 are the masses of the two objects
Reduced Mass Consider two masses m1 and m2
located distances of r1 and r2 from the center of mass of the system
We can define the reduced mass,
= m1m2/(m1+m2)
r1 = -(/m1)rr2 = (/m2)r
Can think of as the reduced mass () orbiting the total mass (M)
Angular Momentum
Orbiting objects have angular momentum In general:
e.g., a single mass, m in a circular orbit of
radius, r:
so for two bodies, total L is:
L = m1r1v1 + m2r2v2
L = [GMa(1-e2)]½
Velocity
Energy of reduced mass
The total system energy is then:
E = -(Gm1m2/2a)
v2 = GM[(2/r)-(1/a)]
Visual Binaries Consider a binary star composed
of two masses in two elliptical orbits around the center of mass (cm)
m1/m2 = a2/a1
1 = a1/d
m1/m2 = 2/1
even if we don’t know the distance, if we can measure ’s we can find the mass ratio
cm
Finding Mass
If we do know the distance, we can get a1 and a2
P2 = (42a3)/[G(m1+m2)]
Have to use m1+m2 and m1/m2 to pull out m’s separately
Inclination
The observed subtended angle is now
ά = cos i then a = d = άd/cos i
m1+m2 = (42/G)(d/cos i)3(ά3/P2)
Next Time
Read: 7.2-7.3 Homework: 2.6, 2.14, 7.4, 7.7, 7.12,