GLIMPSE 70

(Mercer 70; Ryu 273)

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0.21 UTI
0.5
CN
0.26
Cdens
0.38
CC3
0.0
Clit
0.9
Cdup
Radius (P>50% members) 7.8 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.26 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.9 Very likely unique

Overview

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GLIMPSE 70 is a moderately populated, 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 very 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=0.9) 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 – 240.139 -52.163 0.369 -5.002 -4.118 -23.134
Bica et al. 2019 240.123 -52.182 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 70 10.0 240.12 -52.18 0.31 -4.34 -4.26 -42.09 0.32

💡 Note: The % column shows the percentage of members that GLIMPSE 70 shares with each listed object.

Visualization

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