Ruprecht 98
(VDBH 125; MWSC 1988; OCL 868; vdBergh-Hagen 125; ESO 094 09; OCSN 260)
0.90
UTI
0.76
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
31.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Ruprecht 98 is a rich, very dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 179.715 | -64.603 | 2.098 | -4.138 | -8.61 | -5.702 |
| Li et al. | 2025 | 179.715 | -64.581 | 2.044 | -4.114 | -8.632 | â |
| Wei et al. | 2025 | 179.723 | -64.581 | 2.103 | -4.119 | -8.604 | â |
| Almeida et al. | 2025 | 179.842 | -64.505 | â | â | â | â |
| Alfonso et al. | 2024 | 179.564 | -64.451 | 2.054 | -4.251 | -8.52 | â |
| Hunt & Reffert | 2024 | 179.711 | -64.613 | 2.078 | -4.304 | -8.476 | -7.599 |
| Cavallo et al. | 2024 | 179.068 | -64.413 | 2.081 | â | â | â |
| Hunt & Reffert | 2023 | 179.711 | -64.613 | 2.078 | -4.304 | -8.476 | -7.599 |
| Almeida et al. | 2023 | 179.899 | -64.474 | â | â | â | â |
| Qin et al. | 2023 | 179.77 | -64.6 | 2.11 | -4.0 | -8.66 | -5.75 |
| Just et al. | 2023 | 179.707 | -64.584 | â | â | â | â |
| He et al. | 2022 | 179.892 | -64.6 | 2.103 | -4.116 | -8.648 | â |
| Tarricq et al. | 2022 | 179.639 | -64.598 | 2.105 | -4.108 | -8.64 | â |
| Jaehnig et al. | 2021 | 179.681 | -64.609 | 2.068 | -4.209 | -8.724 | â |
| Rain et al. | 2021 | 179.715 | -64.581 | 2.044 | -4.114 | -8.632 | â |
| Dias et al. | 2021 | 179.842 | -64.505 | 2.057 | -4.094 | -8.645 | -4.3 |
| Cantat-Gaudin et al. | 2020 | 179.715 | -64.581 | 2.044 | -4.114 | -8.632 | â |
| Cantat-Gaudin & Anders | 2020 | 179.715 | -64.581 | 2.044 | -4.114 | -8.632 | â |
| Bossini et al. | 2019 | 179.715 | -64.581 | â | â | â | â |
| Soubiran et al. | 2018 | 179.715 | -64.581 | â | â | â | -5.09 |
| Bica et al. | 2019 | 179.68 | -64.575 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 179.715 | -64.581 | 2.044 | -4.114 | -8.632 | â |
| Loktin & Popova | 2017 | 179.67 | -64.583 | â | -10.352 | -3.691 | -7.6 |
| Kharchenko et al. | 2016 | 179.707 | -64.584 | â | â | â | â |
| Dias et al. | 2014 | 179.667 | -64.583 | â | -5.24 | -1.32 | â |
| Kharchenko et al. | 2013 | 179.715 | -64.588 | â | -5.43 | -9.02 | -7.6 |
| Gozha et al. | 2012 | 179.667 | -64.583 | â | â | â | â |
| Piskunov et al. | 2008 | 179.658 | -64.573 | â | â | â | â |
| Kharchenko et al. | 2007 | 179.67 | -64.58 | â | 0.35 | â | -7.6 |
| Piskunov et al. | 2007 | 179.658 | -64.573 | â | â | â | â |
| van den Bergh | 2006 | 179.65 | -64.558 | â | â | â | â |
| Kharchenko et al. | 2005 | 179.67 | -64.58 | â | -5.08 | -9.55 | â |
| Kharchenko et al. | 2003 | 179.61 | -64.54 | â | -4.77 | -10.95 | â |
| Dias et al. | 2002 | 179.667 | -64.583 | â | -7.25 | -7.1 | -7.6 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.45 | 0.48 | â | 826 | -0.150 | â | â | â |
| Wei et al. | 2025 | 0.48 | 0.81 | â | 316 | 0.000 | 203 | 0.44 | â |
| Almeida et al. | 2025 | 0.48 | 0.70 | â | 467 | â | 161 | â | â |
| Alfonso et al. | 2024 | 0.51 | 0.36 | â | 836 | -0.048 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 118* | â | â |
| Cavallo et al. | 2024 | 0.47 | 0.82 | â | 331 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.45 | 0.56 | 1.40 | 244 | â | â | â | â |
| Almeida et al. | 2023 | 0.46 | 0.77 | â | 514 | -0.127 | 259* | 0.53 | â |
| Qin et al. | 2023 | 0.57 | 0.53 | â | 708 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 32 | â | â |
| He et al. | 2022 | â | 0.85 | â | 355 | â | â | â | â |
| Tarricq et al. | 2022 | 0.50 | â | â | 501 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.48* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.48 | 0.50 | â | 316 | â | â | â | 0 |
| Dias et al. | 2021 | 0.48 | 0.70 | â | 467 | -0.049 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.51 | 0.36 | â | 490 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.48 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.47 | 0.50 | â | 570 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.48 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.48 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.64 | 0.51 | â | 313 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.61 | 0.50 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.61 | 0.50 | â | 631 | â | â | â | â |
| Gozha et al. | 2012 | 0.49 | â | â | 322 | â | 263 | â | â |
| Piskunov et al. | 2008 | 0.61 | 0.50 | â | 603 | â | 194* | â | â |
| Piskunov et al. | 2007 | 0.61 | 0.50 | â | 603 | â | 84 | â | â |
| van den Bergh | 2006 | 0.49 | 0.50 | â | 324 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.61 | 0.50 | â | 603 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.49 | 0.62 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.49 | 0.50 | â | 322 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.