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Saturday, 17 January 2026

The Local Hot Bubble (LHB) : Our Solar System’s Superheated Galactic Neighborhood

A Million-Degree Echo of Long-Dead Stars

Written by: L.W (Independent Science Communicator)
Published: 17 January 2026 by Astrophyzix.com

Local hot bubble explained

Introduction 

The Solar System is not drifting through empty, featureless space. Instead, it resides inside a vast, invisible cavity known as the Local Hot Bubble (LHB), a region of unusually hot and extremely diffuse interstellar gas that shapes our cosmic environment in subtle but important ways.


A Bubble in the Interstellar Medium

The Local Hot Bubble is a large cavity within the interstellar medium extending roughly 300 to 1,000 light-years across, depending on direction. Unlike the colder, denser gas clouds that fill much of the Milky Way, the LHB contains plasma heated to temperatures of around one million kelvin, yet with densities so low that it remains effectively a near-vacuum.

Despite its immense temperature, the bubble would feel colder than outer space if you were inside it, simply because there are so few particles present. On average, the LHB contains only about 0.005 atoms per cubic centimetre, far emptier than the best vacuums produced on Earth.


Violent Origins: A Chain of Supernovae

Astronomers believe the Local Hot Bubble formed between 10 and 20 million years ago, carved out by a sequence of nearby supernova explosions. These explosions likely originated from massive stars in the Scorpius–Centaurus OB association, a stellar group that once passed near our region of the Galaxy.

Each supernova blasted away cooler gas and dust while injecting enormous amounts of energy into the surrounding space. Over time, overlapping shock waves merged, excavating a giant cavity and filling it with superheated plasma. Rather than being a single explosion, the LHB is best understood as the fossil imprint of multiple stellar deaths.


How Astronomers Detect an Invisible Structure

The Local Hot Bubble cannot be seen directly, but its presence is revealed through several observational clues:

  • Soft X-ray background radiation, first detected in the 1970s, originating from hot plasma surrounding the Solar System
  • Ultraviolet absorption lines in the spectra of nearby stars, showing where cooler gas begins beyond the bubble
  • 3D dust and hydrogen maps, which outline the bubble’s irregular edges like walls around a cosmic cavity
Local hot bubble graph


Together, these observations confirm that the Sun sits inside a genuine interstellar void rather than a random low-density patch of space.

Our Place Inside the Bubble

While the Solar System resides inside the Local Hot Bubble, it is currently passing through a small, cooler cloud known as the Local Interstellar Cloud. This cloud floats within the bubble like mist inside a vast chamber. Beyond the LHB, astronomers have identified neighboring cavities and tunnels, suggesting the bubble is part of a larger network of connected structures sometimes referred to as a local galactic chimney, venting hot gas toward the Milky Way’s halo.

Traces of Stellar Explosions on Earth

Remarkably, the supernovae responsible for the Local Hot Bubble may have left detectable fingerprints on Earth. Scientists have discovered traces of iron-60, a radioactive isotope produced in supernova explosions, preserved in deep-ocean sediments and lunar samples. These findings suggest that at least one nearby supernova showered the Solar System with debris within the last few million years.

Why the Local Hot Bubble Matters

Understanding the Local Hot Bubble is essential for modern astrophysics. It influences how cosmic rays propagate, affects measurements of the X-ray background, and provides a real-world laboratory for studying how stars reshape the Galaxy. Far from being an empty void, the bubble is a reminder that our corner of the Milky Way has been shaped by powerful, long-forgotten stellar events.

The calm night sky above us hides a turbulent past, and the Local Hot Bubble is one of its quiet, lingering echoes.


Sources and references 

Yeung et al. (2024). The SRG/eROSITA diffuse soft X-ray background — I. The Local Hot Bubble in the western Galactic hemisphere

The full paper (open access) with measurements of the LHB’s temperature structure and soft X-ray emission from the eROSITA All-Sky Survey.

https://www.aanda.org/articles/aa/full_html/2024/10/aa51045-24/aa51045-24.html 

DOI: https://doi.org/10.1051/0004-6361/202451045

Image Credit: Gadget360