Related Experiment Video
Updated: Sep 18, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
Precision analysis of NGC 2158 with Gaia DR3
1National Research Institute of Astronomy and Geophysics (NRIAG), Helwan, 11421, Cairo, Egypt. nasser_ahnmed@yahoo.com.
Researchers re-investigated the open star cluster NGC 2158 using Gaia DR3 data and a novel membership probability method. They determined its astrophysical parameters, mass, age, and distance, identifying blue stragglers and eclipsing binaries.
Area of Science:
- * Astronomy and Astrophysics
- * Stellar Clusters
- * Galactic Astronomy
Background:
- * Open star clusters are fundamental for understanding stellar evolution and galactic dynamics.
- * Previous studies of NGC 2158 may have limitations in membership determination and parameter precision.
- * The Gaia Data Release 3 (DR3) provides unprecedented astrometric and photometric data for stellar research.
Purpose of the Study:
- * To re-investigate the open star cluster NGC 2158 using Gaia DR3 data.
- * To develop and apply a new method for evaluating stellar membership probability within the cluster.
- * To precisely determine the astrophysical parameters, kinematics, and population characteristics of NGC 2158.
Main Methods:
- * Utilized Gaia DR3 data for photometric and astrometric information.
- * Employed the pyUPMASK Python package and HDBSCAN algorithms for cluster membership identification.
- * Developed a novel membership probability assessment based on radial shells within the cluster.
- * Applied the King model and PARSEC stellar isochrones for parameter fitting.
- * Used the galpy Python package for kinematic and orbital parameter calculations.
Main Results:
- * Identified 3067 member stars with a total mass of 3216.4 solar masses.
- * Determined the cluster's mean age at 1.95 ± 0.28 Gyr and distance at 3.733 ± 0.36 kpc.
- * Calculated proper motions and parallax, yielding specific values for these parameters.
- * Constructed a two-power-law mass function, deviating from the single Salpeter slope.
- * Detected 17 variable stars, including 11 eclipsing binaries, and identified 62 blue stragglers.
- * Obtained an average radial velocity of 26.1 ± 2.3 km/s for kinematic analysis.
Conclusions:
- * The new membership probability method provides a more refined analysis of NGC 2158.
- * The study precisely characterizes NGC 2158's astrophysical properties, contributing to cluster studies.
- * The identification of blue stragglers and eclipsing binaries offers insights into stellar populations and evolution within the cluster.
- * Kinematic data reveals NGC 2158's motion within the Milky Way galaxy.
Related Concept Videos
Detection of Black Holes
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Kepler's Third Law of Planetary Motion
Kepler's Second Law of Planetary Motion
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
Kepler's First Law of Planetary Motion
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
Reduced Mass Coordinates: Isolated Two-body Problem
Schwarzschild Radius and Event Horizon
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...

