Pickard 87

Click to load Aladin Lite
0.03 UTI
0.0
CN
0.1
Cdens
0.75
CC3
0.0
Clit
0.16
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.16 Likely duplicate

Overview

â„šī¸
Pickard 87 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 37.212 57.294 0.409 -0.369 -1.131 –
Dias et al. 2026 37.221 57.279 0.406 -0.374 -1.118 –

💡 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 99999– 2.2 1.78 – 16 -0.034 – – –
Dias et al. 2026 2.20 1.78 – 16 -0.034 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 192 84.0 37.05 57.16 0.4 -0.43 -1.15 -27.22 0.47
UBC 606 4.0 37.62 57.27 0.41 -0.28 -1.13 – 0.1

💡 Note: The % column shows the percentage of members that Pickard 87 shares with each listed object.

Visualization

â„šī¸