NGC 7510

(MWSC 3706)

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0.98 UTI
0.9
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 491
Radius (P>50% members) 2.9 [arcmin]
  • CN 0.9 Very rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
πŸ“₯ Members πŸ“Š Colab πŸ”¬ Bayestar19 πŸ” CDS πŸ” Simbad πŸ” CDS (Ξ±, Ξ΄) πŸ” Simbad (Ξ±, Ξ΄)

Overview
ℹ️
NGC 7510 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity and mass parameters (see Parameters). It is very well-studied in the literature.
Relatively close Moderate extinction Massive Near-solar metallicity Young

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

Cavallo et al. (2024)
Gold sample.

Data
πŸ” Search references for NGC 7510 in: SciX Simbad
ℹ️
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 347.763 60.576 0.309 -3.647 -2.236 40.397
Almeida et al. 2025 347.769 60.583 – – – –
Hunt & Reffert 2024 347.766 60.572 0.315 -3.635 -2.226 38.378
Celli et al. 2024 347.767 60.579 – – – –
Cavallo et al. 2024 347.824 60.622 0.314 – – –
Hunt & Reffert 2023 347.766 60.572 0.315 -3.635 -2.226 38.378
Almeida et al. 2023 347.775 60.589 – – – –
Just et al. 2023 347.75 60.576 – – – –
Jaehnig et al. 2021 347.763 60.58 0.316 -3.67 -2.174 –
Rain et al. 2021 347.767 60.579 0.286 -3.664 -2.193 –
Dias et al. 2021 347.769 60.583 0.284 -3.65 -2.194 –
Cantat-Gaudin et al. 2020 347.767 60.579 0.286 -3.664 -2.193 –
SΓ‘nchez et al. 2020 347.762 60.57 – -3.793 -2.135 –
Cantat-Gaudin & Anders 2020 347.767 60.579 0.286 -3.664 -2.193 –
Dias et al. 2019 347.767 60.579 0.286 -3.664 -2.193 63.74
Soubiran et al. 2018 347.767 60.579 – – – 63.74
Cantat-Gaudin et al. 2018 347.767 60.579 0.286 -3.664 -2.193 –
Loktin & Popova 2017 347.76 60.57 – -0.666 -0.132 –
Kharchenko et al. 2016 347.75 60.576 – – – –
Dias et al. 2014 347.762 60.57 – -3.59 -0.86 –
Kharchenko et al. 2013 347.757 60.579 – -2.83 -1.46 –
Kharchenko et al. 2012 347.757 60.579 – -2.83 -1.46 –
Piskunov et al. 2008 347.761 60.565 – – – –
van den Bergh 2006 347.75 60.567 – – – –
Kharchenko et al. 2005 347.76 60.57 – -3.63 -0.92 –
Kharchenko et al. 2003 347.8 60.57 – -3.36 -1.37 –
Dias et al. 2002 347.762 60.57 – -3.59 -0.86 –

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 3.04 2.96 – 9 – 1439 – –
Hunt & Reffert 2024 – – – – – 6937* – –
Celli et al. 2024 – – – 20 – 2568 – –
Cavallo et al. 2024 3.12 3.20 – 29 0.580 – – –
Hunt & Reffert 2023 2.90 3.28 2.78 12 – – – –
Almeida et al. 2023 2.95 3.06 – 10 -0.187 2997* 0.73 –
Just et al. 2023 – – – 50 – 160 – –
Jaehnig et al. 2021 3.15* – – – – – – –
Rain et al. 2021 3.18 2.79 – 22 – – – 0
Dias et al. 2021 3.04 2.96 – 9 -0.206 – – –
Cantat-Gaudin et al. 2020 2.94 2.86 – 19 – – – –
Cantat-Gaudin & Anders 2020 3.18 – – – – – – –
Dias et al. 2019 3.50 2.67 – 13 -0.013 – – –
Soubiran et al. 2018 3.18 – – – – – – –
Cantat-Gaudin et al. 2018 3.18 – – – – – – –
Loktin & Popova 2017 2.13 2.65 – 37 – – – –
Kharchenko et al. 2016 2.10 2.94 – 50 – – – –
Kharchenko et al. 2013 2.10 2.94 – 50 – – – –
Kharchenko et al. 2012 2.10 2.94 – 50 – – – –
Piskunov et al. 2008 2.08 2.79 – 17 – – – –
van den Bergh 2006 2.08 2.67 – 38 – – – –
Kharchenko et al. 2005 2.08 2.79 – 17 – – – –
Kharchenko et al. 2003 2.08 2.63 – – – – – –
Dias et al. 2002 3.48 2.79 – 22 – – – –

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

Visualization
ℹ️
NGC 7510 UCC
NGC 7510 HUNT23
NGC 7510 CANTAT20
Galactocentric position diagram