Local Bubble
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Local Bubble
Local Bubble
Superbubble
Local bubble.jpg
Artist's conception of the Local Bubble (containing the Sun and Beta Canis Majoris) and the Loop I Bubble (containing Antares)
Observation data
Distancely   (0 pc)
Physical characteristics
Radius150 ly
DesignationsLocal Hot Bubble, LHB,[1] Local Bubble, Local Interstellar Bubble[2]
See also: Lists of nebulae
Map showing the Sun located near the edge of the Local Interstellar Cloud and Alpha Centauri about 4 light-years away in the neighboring G-Cloud complex

The Local Bubble, or Local Cavity,[3] is a relative cavity in the interstellar medium (ISM) of the Orion Arm in the Milky Way. It contains among others, the Local Interstellar Cloud, which contains the Solar System, and the G-Cloud. It is at least 300 light years across and is defined by its neutral-hydrogen density of about 0.05 atoms/cm3, or approximately one tenth of the average for the ISM in the Milky Way (0.5 atoms/cm3), and one sixth that of the Local Interstellar Cloud (0.3 atoms/cm3).[dubious ][4]

The exceptionally sparse matter, namely gas, of the Local Bubble is the result of supernovae that exploded within the past ten to twenty million years and remains in an excited state, emitting in the X-ray band.[5][6] It was once thought that the most likely candidate for the remains of this supernova was Geminga, a pulsar in the constellation Gemini. Later, however, it has been suggested that multiple supernovae in subgroup B1 of the Pleiades moving group were more likely responsible,[7] becoming a remnant supershell.[8]

Description

Model of Local Bubble (white), molecular clouds (magenta) & Loop I Bubble (cyan).

The Solar System has been traveling through the region currently occupied by the Local Bubble for the last five to ten million years.[5] 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 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".[9] 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. [10]

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.[11] 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[12].

See also

References

  1. ^ Roland J. Egger, Bernd Aschenbach (February 1995). "Interaction of the Loop I supershell with the Local Hot Bubble". Astronomy and Astrophysics. 294 (2): L25-L28. arXiv:astro-ph/9412086. Bibcode:1995A&A...294L..25E.
  2. ^ "NAME Local Bubble". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2014.
  3. ^ 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
  4. ^ "Our Local Galactic Neighborhood, NASA". Interstellar.jpl.nasa.gov. 2000-02-08. Retrieved .
  5. ^ a b Local Chimney and Superbubbles, Solstation.com
  6. ^ NASA-funded X-ray Instrument Settles Interstellar Debate, www.nasa.gov
  7. ^ T. W. Berghoefer; D. Breitschwerdt (2002). "The origin of the young stellar population in the solar neighborhood - a link to the formation of the Local Bubble?". Astronomy and Astrophysics. 390 (1): 299-306. arXiv:astro-ph/0205128v2. Bibcode:2002A&A...390..299B. doi:10.1051/0004-6361:20020627.
  8. ^ J. R. Gabel, F. C. Bruhweiler (8 January 1998). "[51.09] Model of an Expanding Supershell Structure in the LISM". American Astronomical Society. Retrieved .
  9. ^ Lallement, R.; Welsh, B. Y.; Vergely, J. L.; Crifo, F.; Sfeir, D. (2003). "3D mapping of the dense interstellar gas around the Local Bubble". Astronomy and Astrophysics. 411 (3): 447-464. Bibcode:2003A&A...411..447L. doi:10.1051/0004-6361:20031214.
  10. ^ Koll, D.; et., al. (2019). "Interstellar 60Fe in Antarctica". Physical Review Letters. 123 (7): 072701. doi:10.1103/PhysRevLett.123.072701. PMID 31491090.
  11. ^ "CHIPS - Berkeley University". Chips.ssl.berkeley.edu. 2003-01-12. Archived from the original on 2013-11-21. Retrieved .
  12. ^ 3D map of the local bubble

Further reading

External links


  This article uses material from the Wikipedia page available here. It is released under the Creative Commons Attribution-Share-Alike License 3.0.

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