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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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