NGC 3324 Gabriela Mistral Nebula and the Pearl Cluster

 Posted: May 4th, 2026
Show astrometry on hover
NGC
IC
HD
Technical Info
Telescope/Lens: 250мм Ньютон 1/4
Camera: QHY268M
Mount: Sky-Watcher AZ-EQ6 GT
Guide Scope: QHY off-axis guider
Guide Camera: Lodestar
Software: N.I.N.A, PHD, Pixinsight
Exposure:
275 x 300" ISO/Gain: 25 - LRGBHaOIII
Black, Bortle 1 zone:
 Astrohosting Izabis, Namibia
 Mar 20th, 2026
22 h 55 m
35
Resolution: 6080x4053 px
Scale: 45391 KB

The Gabriela Mistral Nebula is part of the Eta Carinae Nebula complex in the constellation Vela, one of the brightest nebula complexes in the southern sky. It is named after the Chilean poet, as it resembles her profile. Located 7,500 light-years from Earth, it is an active star-forming region. It is primarily an emission nebula in hydrogen and oxygen lines. Its bright pattern is shaped by radiation and stellar winds from hot young stars, which have carved a cavity in the gas and dust, causing the nebula to glow and resemble a human face profile.

The Pearl cluster is an open cluster, NGC 3293, in the constellation Carina. It is young and very rich in bright blue stars. It lies about 8,000–8,400 light-years away and stands out beautifully against the gas and dust regions of the Carina complex, which is why it is often considered one of the most striking southern open clusters.

Add comment

Comments

There are no comments on this picture yet

Comments are available only to registered users. Register or log in to leave a comment.