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Created page with "{{Night Sky | image = | designation =HH-32 | rightascension =19<sup>h</sup> 20<sup>m</sup> 30<sup>s</sup> | declination =+11° 02′ 00″ | distance..."
{{Night Sky
| image =
| designation =HH-32
| rightascension =19<sup>h</sup> 20<sup>m</sup> 30<sup>s</sup>
| declination =+11° 02′ 00″
| distance =1,000 ly
| constellation =[[Aquila]]
| type =[[Herbig–Haro object]]
| dimensions =
| magnitude =
| redshift =
| radvelocity =
| propmotion =
| parallax =
}}
'''HH-32''' is a [[Herbig–Haro object]] found in the [[constellation]] of [[Aquila]].<ref>[http://hubblesite.org/image/902/news/3-nebulae HH 32] from hubblesite.org</ref> It is the green/blue nebula at the top of the image. It is formed when jets of [[gas]] from the [[star]] hit other gas and [[dust]] that produce shockwaves in the gas.<ref name=annesastronomynews.com>[http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/herbig-haro-32-hh-32/ Herbig-Haro 32] from annesastronomynews.com</ref> This creates [[heat]], which causes [[hydrogen]] [[atom]]s to glow green and [[sulfur]] atoms to glow blue.
==Properties and Structure==
The star at the centre of this Herbig-Haro object is catalogued as AS 353A.<ref name=annesastronomynews.com/> The jets are almost aligned along our line of sight, with the length of the two jets totalling around 0.54 [[light year]]s. The jet closest to us is about 0.2 light years long and bi=righter than the other. This may be because the other jet is ejecting less material or it is obscured by gas and dust surrounding the star.
==References==
{{reflist}}
{{Nebulae}}
[[Category:Astronomy]]
[[Category:Nebulae]]
| image =
| designation =HH-32
| rightascension =19<sup>h</sup> 20<sup>m</sup> 30<sup>s</sup>
| declination =+11° 02′ 00″
| distance =1,000 ly
| constellation =[[Aquila]]
| type =[[Herbig–Haro object]]
| dimensions =
| magnitude =
| redshift =
| radvelocity =
| propmotion =
| parallax =
}}
'''HH-32''' is a [[Herbig–Haro object]] found in the [[constellation]] of [[Aquila]].<ref>[http://hubblesite.org/image/902/news/3-nebulae HH 32] from hubblesite.org</ref> It is the green/blue nebula at the top of the image. It is formed when jets of [[gas]] from the [[star]] hit other gas and [[dust]] that produce shockwaves in the gas.<ref name=annesastronomynews.com>[http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/herbig-haro-32-hh-32/ Herbig-Haro 32] from annesastronomynews.com</ref> This creates [[heat]], which causes [[hydrogen]] [[atom]]s to glow green and [[sulfur]] atoms to glow blue.
==Properties and Structure==
The star at the centre of this Herbig-Haro object is catalogued as AS 353A.<ref name=annesastronomynews.com/> The jets are almost aligned along our line of sight, with the length of the two jets totalling around 0.54 [[light year]]s. The jet closest to us is about 0.2 light years long and bi=righter than the other. This may be because the other jet is ejecting less material or it is obscured by gas and dust surrounding the star.
==References==
{{reflist}}
{{Nebulae}}
[[Category:Astronomy]]
[[Category:Nebulae]]