Everything about The Local Bubble totally explained
The
Local Bubble is a cavity in the
interstellar medium (ISM) of the
Orion Arm of the
Milky Way. It is at least 300
light years across and has a neutral
hydrogen density approximately one tenth of the 0.5
atoms per cubic centimetre average for the ISM in the
Milky Way. The hot diffuse gas in the Local Bubble emits
X-rays.
The
Solar System has been travelling through the Local Bubble for the last 3 million years. Its current location lies in the
Local Interstellar Cloud or Local Fluff, a minor region of denser material within the Bubble. The cloud formed where the Local Bubble and the Loop I Bubble met. The gas within the LIC has a density of approximately 0.1 atoms per cubic centimeter.
Most astronomers believe that the Local Bubble was formed between some hundreds of thousands to a few million years ago by nearby
supernovae that pushed aside gas and dust in the local ISM, leaving behind hot, low density material. The most likely candidate for the remains of this supernova is
Geminga, a
pulsar in the
constellation Gemini.
The Local Bubble isn't spherical, but seems to be narrower in the
galactic plane, becoming somewhat egg-shaped or elliptical, and may widen above and below the galactic plane, becoming shaped like an hourglass.
The Local Bubble abuts other bubbles of less dense ISM, including, in particular, the
Loop I Bubble. The Loop I Bubble was created by supernovae and
stellar winds in the
Scorpius-Centaurus Association, some 500 light years from the
Sun. Other bubbles abutting the Local Bubble are the
Loop II Bubble and the
Loop III Bubble.
The Loop I Bubble contains star
Antares (also known as Alpha Scorpii) as shown on the diagram above right.
Further Information
Get more info on 'Local Bubble'.
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