NASA’s Hubble Traces Dark Matter in Dwarf Galaxy Using Stellar Motions

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NASA’s Hubble Traces Dark Matter in Dwarf Galaxy Using Stellar Motions

Draco Dwarf Spheroidal
NASA, ESA, Eduardo Vitral, Roeland van der Marel, and Sangmo Tony Sohn (STScI), DSS; Image processing: Joseph DePasquale (STScI)

What Mystery Does Dark Matter Hold?

The enigmatic qualities and behavior of dark matter, often referred to as the invisible "glue" of the universe, continue to puzzle scientists. Despite being a major component of galaxies, understanding its distribution within a galaxy can provide significant insights into what this elusive substance is and how it influences galactic evolution.

What Does Hubble's Data Reveal About Dark Matter?

A team of astronomers utilized the NASA/ESA Hubble Space Telescope to measure the dynamic motions of stars within the Draco dwarf galaxy, located approximately 250,000 light-years from Earth. By analyzing Hubble observations spanning 18 years, they built the most accurate three-dimensional map of stellar movements within this dwarf galaxy. This unprecedented data helps to shed light on the mysterious qualities and behavior of dark matter.

How Are Stellar Movements Measured?

To understand dark matter within a galaxy, scientists observe the motions of its stars, which are influenced by dark matter's gravitational pull. The Doppler Effect is commonly used to measure the speed of objects moving towards or away from Earth. However, stars also move across the sky, known as proper motion. By combining line-of-sight velocity with proper motions, the team created a comprehensive analysis of the stars’ three-dimensional movements.

Why Focus on the Draco Dwarf Galaxy?

Dwarf galaxies, with their high dark matter content, are ideal subjects for such studies. The team honed in on the Draco dwarf galaxy, a small spheroidal satellite of the Milky Way. The extensive baseline of Hubble observations allowed the team to measure the stars' proper motions with great precision, equivalent to observing an annual shift slightly less than the width of a golf ball seen from the Moon.

What Are the Findings and Implications?

The team discovered that their models aligned more with a cusp-like dark matter structure, supporting cosmological models. These findings provide a deeper understanding of dark matter distribution in galaxies. The methodologies and models developed can be applied to other galaxies, potentially revealing more about the nature of dark matter across different galactic environments.

What’s Next in Dark Matter Research?

The team plans to apply their methods to other dwarf galaxies like Sculptor and Ursa Minor. Future space missions, such as NASA's Nancy Grace Roman Space Telescope, will further investigate dark matter properties by surveying large areas of the sky. This long-term study exemplifies the collaborative effort and patience required to unlock the mysteries of dark matter.

These results, accepted for publication in The Astrophysical Journal, highlight the enduring significance of the Hubble Space Telescope. Operating for over three decades, Hubble continues to make groundbreaking discoveries that enhance our understanding of the universe. Hubble is a collaborative project between NASA and the European Space Agency (ESA), managed by NASA's Goddard Space Flight Center.

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