Planetary Nebulae Codexery

Little Ghost Nebula

A faint, round planetary nebula in Ophiuchus.

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The Little Ghost Nebula, also known as NGC 6369, is a planetary nebula located in the constellation Ophiuchus. It is notable for its round, planet-shaped appearance and relatively faint glow, with a main ring structure about one light-year across. The nebula's light is emitted when high-energy radiation from its central white dwarf excites surrounding atoms of oxygen, hydrogen, and nitrogen, producing blue, green, and red colors respectively.

Quick Facts

Designation
NGC 6369
Constellation
Ophiuchus
Discoverer
William Herschel
Discovery year
1784
Central star spectral type
[WO3]
Main ring diameter
about one light-year

Facts from the source article.

Background

The Little Ghost Nebula was discovered by William Herschel in 1784. It is described as round and planet-shaped, and relatively faint.

The nebula's central star is a white dwarf with a spectral type of [WO3], indicating a spectrum similar to an oxygen-rich Wolf–Rayet star. An analysis of Gaia data suggests that the central star may be a binary system, though it was monitored by the Kepler space telescope and found not to be variable. The nebula's main ring structure is about a light-year across, and its glow comes from ionized oxygen (blue), hydrogen (green), and nitrogen (red).

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Test yourself

Three questions drawn from this entry’s sources. Pick an answer to check it.

1. In which constellation is Little Ghost Nebula located?

Correct.

Not quite. The answer is Ophiuchus.

From the source: “Little Ghost Nebula, also known as NGC 6369, is a planetary nebula in the constellation Ophiuchus.”

2. Who discovered Little Ghost Nebula?

Correct.

Not quite. The answer is William Herschel.

From the source: “It was discovered by William Herschel in 1784.”

3. In what year was Little Ghost Nebula discovered?

Correct.

Not quite. The answer is 1784.

From the source: “It was discovered by William Herschel in 1784.”

Answers checked against the source article

Sources

Compiled from Wikipedia and the sources listed below. Text from Wikipedia is available under CC BY-SA 4.0; this entry is adapted from it.

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