Majaess 88
0.59
UTI
0.7
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
7.2 [N/pc2]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
đĨ Members
đ Colab
đŦ Bayestar19
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
MOCA
đ CDS
đ Simbad
đ CDS (Îą, δ)
đ Simbad (Îą, δ)
Overview
Majaess 88 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 110.979 | -25.87 | 0.762 | -2.672 | 3.285 | 38.552 |
| Hunt & Reffert | 2024 | 110.988 | -25.887 | 0.765 | -2.666 | 3.288 | 34.149 |
| Cavallo et al. | 2024 | 110.949 | -25.778 | 0.763 | â | â | â |
| Hunt & Reffert | 2023 | 110.988 | -25.887 | 0.765 | -2.666 | 3.288 | 34.149 |
| Dias et al. | 2002 | 111.029 | -25.899 | â | -7.28 | 15.9 | â |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.325 | 0.685 | 1.42 | 26 | 0.080 | 132 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 132(1) | â | â |
| Cavallo et al. | 2024 | 1.40 | 0.63 | â | 17 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.25 | 0.74 | 1.42 | 35 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
Palma et al. (2025)
Part of multiple system G216, along with NGC_2362 and Theia_3099.
Cavallo et al. (2024)
Silver sample.