King 17

(MWSC 474; OCL 424)

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0.89 UTI
0.72
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.72 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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King 17 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 parameter (see Parameters). It is very well-studied in the literature.
Distant Moderate extinction Near-solar metallicity Intermediate age

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

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 – 77.09 39.071 0.245 -0.181 -1.377 2.545
Almeida et al. 2025 77.081 39.066 – – – –
Zhang et al. 2024 77.094 39.071 – – – –
Hunt & Reffert 2024 77.094 39.071 0.239 -0.207 -1.409 7.933
Cavallo et al. 2024 77.085 39.06 0.24 – – –
Hunt & Reffert 2023 77.094 39.071 0.239 -0.207 -1.409 7.933
Almeida et al. 2023 77.08 39.069 – – – –
Just et al. 2023 77.09 39.08 – – – –
Dias et al. 2021 77.081 39.066 0.232 -0.112 -1.24 –
Cantat-Gaudin et al. 2020 77.09 39.069 0.239 -0.126 -1.274 –
Cantat-Gaudin & Anders 2020 77.09 39.069 0.239 -0.126 -1.274 –
Soubiran et al. 2018 77.09 39.069 – – – -10.85
Bica et al. 2019 77.1 39.085 – – – –
Cantat-Gaudin et al. 2018 77.09 39.069 0.239 -0.126 -1.274 –
Loktin & Popova 2017 77.085 39.08 – -1.425 0.193 –
Kharchenko et al. 2016 77.09 39.08 – – – –
Dias et al. 2014 77.092 39.069 – 1.63 -1.07 –
Kharchenko et al. 2013 77.1 39.08 – -5.74 0.76 –
Kharchenko et al. 2012 77.1 39.08 – -5.74 0.76 –
Dias et al. 2002 77.092 39.069 – 1.63 -1.07 –

💡 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 3.27 1.74 – 402 – 394 – –
Zhang et al. 2024 – – – – -0.157* – – –
Hunt & Reffert 2024 – – – – – 647* – –
Cavallo et al. 2024 3.21 1.57 – 275 -0.190 – – –
Hunt & Reffert 2023 3.76 1.32 0.57 284 – – – –
Almeida et al. 2023 3.32 1.88 – 36 -0.263 281* 0.61 –
Just et al. 2023 – – – 71 – 482 – –
Dias et al. 2021 3.27 1.74 – 402 -0.285 – – –
Cantat-Gaudin et al. 2020 4.11 1.61 – 52 – – – –
Cantat-Gaudin & Anders 2020 3.73 – – – – – – –
Soubiran et al. 2018 3.73 – – – – – – –
Cantat-Gaudin et al. 2018 3.73 – – – – – – –
Loktin & Popova 2017 3.29 0.75 – 617 – – – –
Kharchenko et al. 2016 3.00 2.17 – 71 – – – –
Kharchenko et al. 2013 3.00 2.17 – 71 – – – –
Kharchenko et al. 2012 3.00 2.17 – 71 – – – –
Dias et al. 2002 4.71 1.74 – 251 – – – –

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

Visualization

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