Gomez's Hamburger
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Gomez's Hamburger, also known as IRAS 18059-3211 or Gomez's Whopper is an astronomical object believed to be a young A-type star surrounded by a
protoplanetary disk A protoplanetary disk is a rotating circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may not be considered an accretion disk; while the two are sim ...
. It was initially identified as a
planetary nebula A planetary nebula is a type of emission nebula consisting of an expanding, glowing shell of ionized gas ejected from red giant stars late in their lives. The term "planetary nebula" is a misnomer because they are unrelated to planets. The ...
, and its distance was estimated to be approximately 6500
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away from
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. However, recent results suggest that this object is a young star surrounded by a
protoplanetary disk A protoplanetary disk is a rotating circumstellar disc of dense gas and dust surrounding a young newly formed star, a T Tauri star, or Herbig Ae/Be star. The protoplanetary disk may not be considered an accretion disk; while the two are sim ...
, at a distance of about 900 light-years away. It was discovered in 1985 on sky photographs obtained by Arturo Gómez, support technical staff at the
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near
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,
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. The photos suggested that there was a dark band across the object, but its exact structure was difficult to determine because of the atmospheric turbulence that hampers all images taken from the ground. The star itself has a surface temperature of approximately 10,000 K. The "buns" are light reflecting off dust. A disk of dust seen nearly exactly edge-on obscures the star and produces the dark band in the middle, the "burger". It has a dim visual magnitude of 14.4.


Possible protoplanet

An emission at the southern part of the disk seen in
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imaging, as well as in mid-infrared imaging, was interpreted as a
protoplanet A protoplanet is a large planetary embryo that originated within a protoplanetary disk and has undergone internal melting to produce a differentiated interior. Protoplanets are thought to form out of kilometer-sized planetesimals that gravitatio ...
candidate, termed GoHam b. This candidate would have a mass of 0.8-11.4 . Protoplanetary disk can however form disk fragments that are gravitationally bound and can mimic protoplanets. In the case of GoHam b it is not clear if it is a protoplanet or just a disk fragment.


Gallery

File:GoHam JWST NIRCam.jpg, JWST NIRCam image of GoHam File:GoHam JWST MIRI.jpg, JWST MIRI image of GoHam File:GoHam decaps dr2.jpg, Gomez's Hamburger from the ground with DESI legacy surveys


References

{{Sagittarius (constellation) Pre-stellar nebulae Circumstellar disks IRAS catalogue objects Sagittarius (constellation)