dc.contributor.author |
Vyasanakere, Jayanth P |
|
dc.contributor.author |
Bhatnagar, Siddharth |
|
dc.contributor.author |
Murthy, J |
|
dc.date.accessioned |
2021-12-16T04:06:15Z |
|
dc.date.available |
2021-12-16T04:06:15Z |
|
dc.date.issued |
2021-12 |
|
dc.identifier.citation |
Pramana Journal of Physics, Vol. 95, No. 4, 192 |
en_US |
dc.identifier.issn |
0304-4289 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/7886 |
|
dc.description |
Restricted Access |
en_US |
dc.description |
The original publication is available at springerlink.com |
|
dc.description.abstract |
We describe a method that does not use any orbital parameters, to arrive at the position and mass of
a new celestial object, using high-precision orbital state vector data of the rest of the objects in the system. As an
illustration of this approach, we rediscover Neptune with remarkable accuracy. |
en_US |
dc.language.iso |
en |
en_US |
dc.publisher |
Springer |
en_US |
dc.relation.uri |
https://doi.org/10.1007/s12043-021-02238-2 |
|
dc.rights |
© Indian Academy of Sciences |
|
dc.subject |
Non-parametric algorith |
en_US |
dc.subject |
Neptune |
en_US |
dc.subject |
iteration method |
en_US |
dc.title |
Discovering a celestial object using a non-parametric algorithm |
en_US |
dc.type |
Article |
en_US |