| 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 |