IC 1805 & HB3 – Mosaic of the Heart Nebula

IC 1805 & HB3

The Heart Nebula and a Supernova remnant

Energetic light and winds

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First, the large emission nebula dubbed IC 1805 looks, in whole, like a human heart. The nebula glows brightly in red light emitted by its most prominent element: hydrogen. The red glow and the larger shape are all powered by a small group of stars near the nebula’s center. In the center
of the Heart Nebula are young stars from the open star cluster Melotte 15 that are eroding away several picturesque dust pillars with their energetic light and winds. The Heart Nebula is located about 7,500 light years away toward the constellation of Cassiopeia. At the bottom right is HB3,
a faint supernova remnant located nearby that is the result of a massive star’s explosion, which expelled its outer layers into space. This remnant has an elongated, irregular shape and is characterized by diffuse, low surface brightness, making it less conspicuous than some other nebulae.

The Heart Nebula in Cassiopeia

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Technical card

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ObjectIC 1805 / IC 1795 / HB3
Imaging telescopesCelestron Rowe-Ackermann Schmidt Astrograph 11″
Imaging cameraQHY268M
Mount iOptron CEM120
GuidingSkywatcher Evoguide 50ED, QHY174M
FilterBaader 3.5 / 4nm f/2 Ultra-Highspeed-Filter-Set 50mm² (H-alpha / O-III), Baader R, G, B (50mm²)
AccessoriesBaader UFC, Baader UFC-Tilter,  Celestron Focus Motor for SCT
Integration84.25 hours (H-alpha: 520×180″, O-III: 530×180″, SII: 535×180″, RGB each: 200×30″)
Dates of recordingBetween August 2024 and Oktober 2024
AstroBinLink

HEART NEBULA PRINT & RAW DATA

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