Attempted Very Precise 2004 MN4 Apophis orbital elements
Posted: 14.10.2008, 08:30
Hello, I'm new here, this is my first attempt at doing anything. You have to start somewhere. The SSC file is pasted below.
I basically pulled the data from JPL's browser and the rotation period from http://earn.dlr.de/nea/099942.htm. My first question is do people usually source their data, is it legal not to? I wasn't sure so I played on the safe side and put it in. Second off this data works much better than the plugin at the Motherlode (mine gets within the moon's orbit, 269,590 km to be exact), but it still doesn't put it into the error range that is the stated error range for the 2029 pass as stated on wikipedia at http://en.wikipedia.org/wiki/99942_Apophis Is there any other location that gives more precise data such that I can get it within this error range? Also is there any more advanced features for more advanced orbits than just a single elipse. Can we put in separate orbits for different Julian dates such that it slowly changes between them? For example, I'm guessing this error comes in from the fact that this data is for the current date and not for the date for the close approach and it's close passes with other orbital bodies shifts its orbit slightly such that it moves closer, and NASA (and others) takes these into effect. So for example if we gives 20 or so orbits over several years at any time the date will be much closer. Is there a feature to do this other than straight single "EllipticalOrbit" settings in .ssc files (and yes I know about defining xyz for them but that would be quite a large amount of data for one asteroid.) It could also come from how exactly Earth's orbit is being calculated in 2029, although I'm guessing you guys have that defined pretty exactly.
Thanks in advance,
Ergzay
# This file contains the orbital elements and some other data for the 99942 Apophis (2004 MN4) Near-Earth Asteroid (NEA)
# Author Matthew Lindner on October 14, 2008.
"2004 MN4" "Sol"
{
Class "asteroid"
Mesh "asteroid.cms"
Texture "asteroid.jpg"
Radius 0.27
EllipticalOrbit
{
Period 0.885920179879516
SemiMajorAxis 0.9224221637574083
Eccentricity 0.1912119299890948
Inclination 3.331425002325445
AscendingNode 204.4451349657969
ArgOfPericenter 126.4064496795719
MeanAnomaly 254.9635275775066
Epoch 2454800.5
}
Albedo 0.33
RotationPeriod 30.5376
}
# Data retrieved from
# JPL Small-Body Database Browser (http://ssd.jpl.nasa.gov/sbdb.cgi) and
# Database of Near-Earth Asteroids (http://earn.dlr.de/nea/099942.htm)
I basically pulled the data from JPL's browser and the rotation period from http://earn.dlr.de/nea/099942.htm. My first question is do people usually source their data, is it legal not to? I wasn't sure so I played on the safe side and put it in. Second off this data works much better than the plugin at the Motherlode (mine gets within the moon's orbit, 269,590 km to be exact), but it still doesn't put it into the error range that is the stated error range for the 2029 pass as stated on wikipedia at http://en.wikipedia.org/wiki/99942_Apophis Is there any other location that gives more precise data such that I can get it within this error range? Also is there any more advanced features for more advanced orbits than just a single elipse. Can we put in separate orbits for different Julian dates such that it slowly changes between them? For example, I'm guessing this error comes in from the fact that this data is for the current date and not for the date for the close approach and it's close passes with other orbital bodies shifts its orbit slightly such that it moves closer, and NASA (and others) takes these into effect. So for example if we gives 20 or so orbits over several years at any time the date will be much closer. Is there a feature to do this other than straight single "EllipticalOrbit" settings in .ssc files (and yes I know about defining xyz for them but that would be quite a large amount of data for one asteroid.) It could also come from how exactly Earth's orbit is being calculated in 2029, although I'm guessing you guys have that defined pretty exactly.
Thanks in advance,
Ergzay
# This file contains the orbital elements and some other data for the 99942 Apophis (2004 MN4) Near-Earth Asteroid (NEA)
# Author Matthew Lindner on October 14, 2008.
"2004 MN4" "Sol"
{
Class "asteroid"
Mesh "asteroid.cms"
Texture "asteroid.jpg"
Radius 0.27
EllipticalOrbit
{
Period 0.885920179879516
SemiMajorAxis 0.9224221637574083
Eccentricity 0.1912119299890948
Inclination 3.331425002325445
AscendingNode 204.4451349657969
ArgOfPericenter 126.4064496795719
MeanAnomaly 254.9635275775066
Epoch 2454800.5
}
Albedo 0.33
RotationPeriod 30.5376
}
# Data retrieved from
# JPL Small-Body Database Browser (http://ssd.jpl.nasa.gov/sbdb.cgi) and
# Database of Near-Earth Asteroids (http://earn.dlr.de/nea/099942.htm)