GLIMPSE 83

(Mercer 83)

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0.06 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.0
Clit
0.84
Cdup
Radius (P>50% members) 8.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.84 Very likely unique

Overview

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GLIMPSE 83 is a sparse, very loose object of low 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 7 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=0.84) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 253.378 -43.362 0.425 -2.867 -4.22 -28.31
Bica et al. 2019 253.365 -43.401 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVV 089 16.0 253.48 -43.21 0.44 -2.82 -3.91 -40.06 0.05

💡 Note: The % column shows the percentage of members that GLIMPSE 83 shares with each listed object.

Visualization

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