The exceptionally sparse gas of the Local Bubble is the result of
supernovae that exploded within the past ten to twenty million years.
Geminga, a
pulsar in the
constellation Gemini, was once thought to be the remnant of a single supernova that created the Local Bubble, but now multiple supernovae in subgroup B1 of the
Pleiadesmoving group are thought to have been responsible,[5] becoming a remnant
supershell.[6] Other research suggests that the subgroups Lower Centaurus–Crux (LCC) and Upper Centaurus–Lupus (UCL), of the
Scorpius–Centaurus association created both the local bubble and the Loop I Bubble. With LCC being responsible for the Local Bubble and UCL being responsible for the Loop I Bubble.[7] It was found that 14 to 20 supernovae originated from LCC and UCL, which could have formed these bubbles.[8]
Description
The
Solar System has been traveling through the region currently occupied by the Local Bubble for the last five to ten million years.[9] Its current location lies in the
Local Interstellar Cloud (LIC), a minor region of denser material within the Bubble. The LIC formed where the Local Bubble and the
Loop I Bubble met. The gas within the LIC has a density of approximately 0.3 atoms per cubic centimeter.
The Local Bubble is not 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. It abuts other bubbles of less dense interstellar medium (ISM), including, in particular, the Loop I Bubble. The Loop I Bubble was cleared, heated and maintained by supernovae and
stellar winds in the
Scorpius–Centaurus association, some 500 light years from the
Sun. The Loop I Bubble contains the star
Antares (also known as α Sco, or Alpha Scorpii), as shown on the diagram above right. Several tunnels connect the cavities of the Local Bubble with the Loop I Bubble, called the "Lupus Tunnel".[10] Other bubbles which are adjacent to the Local Bubble are the
Loop II Bubble and the
Loop III Bubble. In 2019, researchers found interstellar iron in Antarctica which they relate to the
Local Interstellar Cloud, which might be related to the formation of the Local Bubble.[11]
Observation
Launched in February 2003 and active until April 2008, a small space observatory called
Cosmic Hot Interstellar Plasma Spectrometer (CHIPS or CHIPSat) examined the hot gas within the Local Bubble.[12] The Local Bubble was also the region of interest for the
Extreme Ultraviolet Explorer mission (1992–2001), which examined hot EUV sources within the bubble. Sources beyond the edge of the bubble were identified but attenuated by the denser interstellar medium. In 2019, the first 3D map of the Local Bubble has been reported using the observations of diffuse interstellar bands.[13]
In 2020, the shape of the dusty envelop surrounding the Local Bubble was retrieved and modeled from 3D maps of the dust density obtained from stellar extinction data.[14]
Impact on star formation
In January 2022, a paper in the journal Nature found that observations and modelling had determined that the action of the expanding surface of the bubble had collected gas and debris and was responsible for the formation of all young, nearby stars.[17]
On
earth several
radioactive isotopes were connected to supernovae occurring relative nearby to the solar system. The most common source is found in deep sea
ferromanganese crusts. Such nodules are constantly growing and deposits iron, manganese and other elements. Samples are divided into layers which are dated for example with
Beryllium-10. Some of these layers have higher concentrations of radioactive isotopes.[18] The isotope most commonly associated with supernovae on earth is
Iron-60 from
deep sea sediments,[19]Antarctic snow,[20] and
lunar soil.[21] Other isotopes are
Manganese-53[22] and
Plutonium-244[18] from deep sea materials. Supernova originated
Aluminium-26, which was expected from cosmic ray studies, was not confirmed.[23] Iron-60 and Manganese-53 have a peak 1.7–3.2 Million years ago and Iron-60 has a second peak 6.5–8.7 Million years ago. The older peak likely originated when the solar system moved through the
Orion-Eridanus superbubble and the younger peak was generated when the solar system entered the local bubble 4.5 Million years ago.[24] One of the supernovae creating the younger peak might have created the pulsar
PSR B1706-16 and turned
Zeta Ophiuchi into a
runaway star. Both originated from UCL and were released by a supernova 1.78 ± 0.21 Million years ago.[25] Another explanation for the older peak is that it was produced by one supernova in the
Tucana-Horologium association 7-9 Million years ago.[26]
^Abt, Helmut A. (December 2015). "Hot gaseous stellar disks avoid regions of low interstellar densities". Publications of the Astronomical Society of the Pacific. 127 (958): 1218–1225.
Bibcode:
2015PASP..127.1218A.
doi:
10.1086/684436.
S2CID124774683.
^"Our local galactic neighborhood". Interstellar.jpl.nasa.gov. National Aeronautics and Space Administration (
NASA). 8 February 2000. Archived from
the original on 21 November 2013. Retrieved 23 July 2013.