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%matplotlib inline
import matplotlib.pyplot as plt
import numpy as np
from astropy.table import QTable
SDSS_MainBelt.csv
contains data on objects in the asteroid belt collected by the Sloan Digital Sky Survey.The columns are:
Name
- Object namea
- semi-major axiscA
- SDSS a$^*$ colorcI
- SDSS i color (near infrared)cZ
- SDSS z color (infrared)X
- X position [au] - Sun-centered coords (10/29/2014)Y
- Y position [au] - Sun-centered coords (10/29/2014)Z
- Z position [au] - Sun-centered coords (10/29/2014)
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P
= a **
(3/2)Pjup
= 11.8618 yearsPjup / P
)Pjup / P
) = 1,2,3,4
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a
) for all of the asteroids.a
< 3.6 AUa
for C-Type asteroids only.a
for S-Type asteroids only.a
for V-Type asteroids only.a
= mean(a
) for that type of asteroid.
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