DOI Serbia časopisi

National library of Serbia

Cobiss

All issues
- 2024 OnLine-First
  - Issue 00
- 2023
  - Issue 207
  - Issue 206
- 2022
  - Issue 205
  - Issue 204
- 2021
  - Issue 203
  - Issue 202
- 2020
  - Issue 201
  - Issue 200
- 2019
  - Issue 199
  - Issue 198
- 2018
  - Issue 197
  - Issue 196
- 2017
  - Issue 195
  - Issue 194
- 2016
  - Issue 193
  - Issue 192
- 2015
  - Issue 191
  - Issue 190
- 2014
  - Issue 189
  - Issue 188
- 2013
  - Issue 187
  - Issue 186
- 2012
  - Issue 185
  - Issue 184
- 2011
  - Issue 183
  - Issue 182
- 2010
  - Issue 181
  - Issue 180
- 2009
  - Issue 179
  - Issue 178
- 2008
  - Issue 177
  - Issue 176
- 2007
  - Issue 175
  - Issue 174
- 2006
  - Issue 173
  - Issue 172
- 2005
  - Issue 171
  - Issue 170
- 2004
  - Issue 169
  - Issue 168
- 2003
  - Issue 167
  - Issue 166
- 2002
  - Issue 165
- 2001
  - Issue 163
  - Issue 164
- 2000
  - Issue 161
  - Issue 162
- 1999
  - Issue 159
  - Issue 160
- 1998
  - Issue 157
  - Issue 158

Serbian Astronomical Journal 2005 Issue 171, Pages: 37-42
https://doi.org/10.2298/SAJ0571037K
Full text ( 205 KB)
Cited by

The mass of (1) Ceres obtained from four close encounters

Kovačević Anđelka B. (Department of Astronomy, Faculty of Mathematics, Belgrade)
Kuzmanoski Mike S. (Department of Astronomy, Faculty of Mathematics, Belgrade)

The technique of asteroid mass determination from perturbation during close approach requires as many as possible different close approaches in order to derive reliable mass of a perturber. Here are presented some results for the mass of (1) Ceres obtained using newly found close approaches.

Keywords: celestial mechanics

doiSerbia