The California Nebula

The California Nebula (NGC1499) is a bright red hydrogen emission nebula located in the Perseus constellation.  Its name comes from its resemblance to the California state. With an apparent magnitude of 5, it is a popular target for amateur astrophotographers using a camera and telescope. Similar nebulae include the North America Nebula, Heart Nebula, and the Rosette Nebula.

Specifications:

Designation: NGC1499

Known As: The California Nebula

Apparent Size: 2.7° x 40′

Magnitude (lower is brighter): 5.0

Distance from Earth: 1,300 LY

Capitalizing on all the Hydrogen

The image above was taken in a Bortle 7 sky using the ZWO Duo-Band Filter. This target doesn’t have too much OIII, being mostly built up of red ionized hydrogen gas clouds.

ACQUISITION
Integration Time: 4.67 hours
RGB: 56x 300sec
BIN: 1×1
Gain: 110
Temperature: -10° C
Bortle Scale: 7

CALIBRATION
Darks: 10
Flats: 20
Offset/Bias: 20

The Perseus Constellation

Perseus (Greek Hero) is located in the north, and has the  Milky Way pass through. The brightest star is the yellow-white star called Mirfak. It also hosts the annual Perseids meteor shower, which is one of the most active meteor showers in the sky. The Perseus constellation is bordered by Aries, Taurus, Auriga,  Camelopardalis, Cassiopeia, Andromeda and Triangulum.

The California Nebula is located in the foot of Perseus, just above the star, Menkib. Other deep sky objects located in the Perseus constellation include: Little Dumbbell Nebula and M34.

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*General information regarding constellations, galaxies, nebulae, and planets have been sourced from: AstroBackyard, VisibleDark, Wikipedia, EarthSky, and NASA.

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