NGC 1348

(MWSC 289; OCL 391; FSR 0650)

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0.90 UTI
0.74
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique

Overview

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NGC 1348 is a moderately populated, very dense 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, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 53.539 51.403 0.439 1.258 -0.775 -24.137
Almeida et al. 2025 53.526 51.414 – – – –
Zhang et al. 2024 53.545 51.4 – – – –
Hunt & Reffert 2024 53.545 51.4 0.442 1.239 -0.775 -19.885
Cavallo et al. 2024 53.495 51.411 0.444 – – –
Hunt & Reffert 2023 53.545 51.4 0.442 1.239 -0.775 -19.885
Just et al. 2023 53.538 51.399 – – – –
Jaehnig et al. 2021 53.543 51.399 0.443 1.276 -0.73 –
Rain et al. 2021 53.524 51.409 0.404 1.288 -0.726 –
Dias et al. 2021 53.526 51.414 0.395 1.312 -0.686 –
Cantat-Gaudin et al. 2020 53.524 51.409 0.404 1.288 -0.726 –
SΓ‘nchez et al. 2020 53.525 51.408 – 1.481 -0.84 –
Cantat-Gaudin & Anders 2020 53.524 51.409 0.404 1.288 -0.726 –
Bica et al. 2019 53.535 51.415 – – – –
Cantat-Gaudin et al. 2018 53.524 51.409 0.404 1.288 -0.726 –
Loktin & Popova 2017 53.52 51.409 – 1.094 -3.514 –
Kharchenko et al. 2016 53.538 51.399 – – – –
Dias et al. 2014 53.525 51.408 – 0.59 -0.45 –
Kharchenko et al. 2013 53.55 51.4 – 1.92 -3.35 –
Gozha et al. 2012 53.525 51.408 – – – –
Kharchenko et al. 2012 53.55 51.4 – 1.92 -3.35 –
Chen et al. 2003 53.522 51.421 – – – –
Dias et al. 2002 53.525 51.408 – 0.59 -0.45 –

πŸ’‘ 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] Bfr BSS
Almeida et al. 2025 2.09 2.84 – 12 – 609 – –
Zhang et al. 2024 – – – – 0.000* – – –
Hunt & Reffert 2024 – – – – – 830* – –
Cavallo et al. 2024 2.54 3.04 – 34 0.640 – – –
Hunt & Reffert 2023 2.05 3.08 2.47 56 – – – –
Just et al. 2023 – – – 282 – 27 – –
Jaehnig et al. 2021 2.24* – – – – – – –
Rain et al. 2021 2.31 3.16 – 129 – – – 0
Dias et al. 2021 2.09 2.84 – 12 -0.197 – – –
Cantat-Gaudin et al. 2020 2.40 2.55 – 42 – – – –
Cantat-Gaudin & Anders 2020 2.31 – – – – – – –
Cantat-Gaudin et al. 2018 2.31 – – – – – – –
Loktin & Popova 2017 1.33 2.93 – 179 – – – –
Kharchenko et al. 2016 1.80 2.63 – 282 – – – –
Kharchenko et al. 2013 1.80 2.63 – 282 0.070 – – –
Gozha et al. 2012 1.82 – – 129 0.070 – – –
Kharchenko et al. 2012 1.80 2.63 – 282 0.070 – – –
Chen et al. 2003 1.82 3.16 – 130 0.070* – – –
Dias et al. 2002 1.82 3.16 – 129 0.070 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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