FSR 1662

(C1341-617; SAI 119)

Click to load Aladin Lite
0.12 UTI
0.0
CN
0.1
Cdens
0.62
CC3
0.0
Clit
0.8
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.8 Very likely unique

Overview

â„šī¸
FSR 1662 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 16 years.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.8) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 206.105 -62.089 0.262 -6.744 -1.857 -39.724
Glushkova et al. 2010 206.059 -62.068 – – – –
Froebrich et al. 2007 206.021 -62.038 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 38 20.0 206.06 -62.03 0.35 -6.75 -2.03 -49.98 0.09

💡 Note: The % column shows the percentage of members that FSR 1662 shares with each listed object.

Visualization

â„šī¸