# PROPERTIES OF INITIAL CONDITIONS 

# The following options are all required; units can contain numbers
# and metric prefixes:

AngleUnit:  deg		# base unit choices: deg, rad
MassUnit:   Msun   	# base unit choices: g, Msun
LengthUnit: AU		# base unit choices: m, AU (or ua), pc
TimeUnit:   yr		# base unit choices: s, h, d, yr

StepSize:   0.01	# integration time step       (units of TimeUnit)

M  =  1   		# mass of the dominant object (units of MassUnit)
N  =  Auto		# number of objects (including the dominant mass)


PostNewtonian: No	# Include leading-order post-Newtonian corrections?

InputOrder: Mass SemiMajorAxis  Eccentricity Inclination \
		 LongAscendNode LongPeriapse  TrueLong

ParticleType: HWP              # Values from Danby, Epoch 2000

1.6601e-7   0.3871  0.205632  7.005  48.33   77.45  252.25    # Mercury
2.4480e-6   0.7233  0.006772  3.395  76.68  131.56  181.98    # Venus
3.0039e-6   1.0000  0.016709   0.00   0.00  102.93  100.47    # Earth
3.2272e-7   1.5237  0.093401  1.850  49.55  336.06  355.43    # Mars


Tfinal  =  50000  		# final integration time (TimeUnit)

OutputFiles: body%d.dat		# name of body-specific output files
OutputOrder: time Semi Ecc Inc LongA LongP TrueLong  	# data columns
OutputInterval: 50.65639	# time interval to write output (TimeUnit)
OutputCoord: Bodycentric	# output coordinate system
OutputHeader: True		# Include column id codes and comments?
OutputDigits: 8			# precision of numbers in output 
OutputTypes: HWPs		# particle types to produce files for