2020 CD3 - new temporary mini moon

I understand looking at Tony Dunn's simulations (press orbit simulator view button in this page provided by Bill Gray's project pluto) and comments in MPML that chaos is playing a big role here.

For this reason, I am not sure that a backward simulation can be useful to get an idea of the asteroid behaviour.
Probably not .. .but just for curiosity let's do it and let's assume for a moment that 2020 CD3 is a natural object.

I generated 100 clones trying to achieve the "same" orbital parameters and sigma as provided by the JPL solution (Horizons Web Interface)

	Clones			Target
	mean	sd		mean	sd
q	1.00502954166	2.714862e-05		1.00503150094	2.7143e-05
e	0.01726251622	2.418728e-05		0.01726090999	2.4152e-05
i	0.6401240941	0.00012806312		0.64011545932	0.0001279
peri	46.79953402529	0.09813338369		46.79424491192	0.098245
node	83.09078802026	0.05641077311		83.08730279228	0.056433
tp	2458877.63623114	0.04030051738		2458877.6339221	0.040361

I gave a look at close encounters with other planets a part Eeath-Moon itself.
It seems that in order to see these hypothetical close encounters we need to go back many centuries.
I found that these encounters are more likely and more recent with Venus rather than Mars.
Could this be a hint that the origin of this object is from the inner part of the solar system?

Kind Regards,
Alessandro Odasso