Ruprecht 53

(MWSC 1442; OCL 682; ESO 494 32)

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0.72 UTI
0.54
CN
0.89
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members) 11.9 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.89 Dense
  • CC3 0.75 High quality
  • Clit 0.7 Moderately studied
  • Cdup 1.0 Unique

Overview

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Ruprecht 53 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~1.03 kpc) differs significantly from the median photometric distance (~1.52 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 122.737 -27.027 0.968 -2.864 1.004 11.48
Hunt & Reffert 2024 122.741 -27.003 0.956 -2.877 0.99 11.802
Cavallo et al. 2024 122.728 -27.037 0.957 – – –
Hunt & Reffert 2023 122.741 -27.003 0.956 -2.877 0.99 11.802
Just et al. 2023 122.674 -26.937 – – – –
Bica et al. 2019 122.717 -26.991 – – – –
Kharchenko et al. 2016 122.674 -26.937 – – – –
Dias et al. 2014 122.725 -27.0 – -2.0 4.52 –
Kharchenko et al. 2013 122.68 -26.94 – -0.34 5.63 –
Piskunov et al. 2008 122.692 -26.993 – – – –
Kharchenko et al. 2005 122.7 -27.0 – -1.11 0.32 –
Kharchenko et al. 2003 122.64 -27.0 – -0.58 0.46 –
Dias et al. 2002 122.725 -26.0 – -2.0 4.52 –

💡 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
Hunt & Reffert 2024 – – – – – 126* – –
Cavallo et al. 2024 1.00 0.19 – 309 -0.070 – – –
Hunt & Reffert 2023 0.97 0.09 0.54 343 – – – –
Just et al. 2023 – – – 724 – 97 – –
Kharchenko et al. 2016 1.52 0.84 – 724 – – – –
Kharchenko et al. 2013 1.52 0.84 – 724 – – – –
Piskunov et al. 2008 1.70 0.34 – 389 – – – –
Kharchenko et al. 2005 1.70 0.34 – 389 – – – –
Kharchenko et al. 2003 1.00 0.46 – – – – – –
Dias et al. 2002 1.70 0.34 – 389 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1026 77.2 122.75 -27.04 0.97 -2.86 1.02 11.15 0.0

💡 Note: The % column shows the percentage of members that Ruprecht 53 shares with each listed object.

Visualization

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