The object called IC 1396, also known as the Elephant Rüsselnebel, is located in the constellation Kepheus and consists of interstellar gas and dust.

The striking dark clouds of dust (globules) are areas where new stars arise. Due to high gravity, the gas is compressed further and further, so the cloud collapses. So-called protosters are emerging, which absorbs more and more gas and dust, until finally nuclear fusion begins and new stars are emerging.

The stars then make the surrounding gas shine.

A total of almost 14 hours of narrowband footage of hydrogen, sulfur and oxygen were taken and processed according to the Hubble color palette.

Hydrogen is green, oxygen is blue and sulphur is red.

This is how the different gases can be presented differently.

Here are some more dates:

- - Skywatcher Newton 200 / 1000

- - PROBABLY 1600 MM

- - Mount: Skywatcher EQ8-R

- - Filter: Ha, S2, O3

- - Guiding: MGEN 2 at Skywatcher Seeker

- - N.I.N.A., APP, Photoshop

- - 90 x 300 Sek (-15°C) - GAIN 139 (Ha)

- - 20 x 600 Sek (-15°C) - GAIN 139 (O3)

- - 35 x 300 Sek (-15°C) - GAIN 139 (S2)

- - Total exposure time: 14 hours

Copyright: Chris K. Fotografie