MCM 77
(MCM2005b 77)
0.11
UTI
0.0
CN
0.36
Cdens
0.25
CC3
0.0
Clit
0.92
Cdup
Stellar density (N50/rad)
1.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.36 Loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.92 Very likely unique
Overview
MCM 77 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.
(*): The parallax distance estimate (~2.74 kpc) differs significantly from the median photometric distance (~6.08 kpc).
Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.92) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 244.333 | -50.53 | 0.364 | -4.076 | -4.087 | -43.497 |
| Morales et al. | 2013 | 244.363 | -50.511 | â | â | â | â |
| Mercer et al. | 2005 | 244.367 | -50.511 | â | â | â | 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 | 6.08 | â | â | â | â | â | â | â |
| Morales et al. | 2013 | 6.08 | â | â | â | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster.
Mercer et al. (2005)
Association of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm.