NGC 1785

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.0 0.25 0.0 1.0
C3
N_50
r_50
CC 6 5.5
Summary

NGC 1785 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 74.646 -68.844 – 3.43 -1.78 9.7
Loktin & Popova (2017) 74.64 -68.843 – -6.041 4.061 9.7
           
UCC 74.696 -68.816 -0.017 1.878 0.075 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

NGC 1785 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.06, Dist=3080.0, Age=8.7
Loktin & Popova (2017) E(B-V)=0.967, Dist=1283, logt=9.2

Search coordinates in Bayestar19

Cluster region map