Jet from Young Star

This arrowhead structure is a classic bowshock pattern produced when high-speed material encounters a slower-speed medium. Young stellar jets were discovered 20 years ago, in part due to visible-light observations of bright patches of nebulosity (called Herbig-Haro objects), which appear to be moving away from associated protostars.

Credit:

J. Hester (Arizona State University), the WFPC 2 Investigation Definition Team, and NASA/ESA

About the Image

NASA press release
Id:opo9524h
Type:Observation
Release date:6 June 1995, 20:00
Size:230 x 268 px

About the Object

Name:HH 1, HH 2
Type:Milky Way : Star : Evolutionary Stage : Young Stellar Object
Milky Way : Nebula : Type : Jet
Constellation:Orion
Category:Stars

Image Formats

r.titleLarge JPEG
45.4 KB
r.titleScreensize JPEG
259.1 KB

Coordinates

Position (RA):5 36 20.49
Position (Dec):-6° 45' 18.45"
Field of view:0.38 x 0.44 arcminutes
Orientation:North is 18.5° right of vertical


Colours & filters

BandTelescope
Hubble Space Telescope
WFPC2

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