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EntityQ947975· pop 36· linked from 437 articles

planetary nebula

In the Vinony graph

Within Vinony's link graph, NGC 6210 is referenced by 437 other articles, and connects out to list of NGC objects (6001–7000), Lagoon Nebula and epoch.

It is catalogued under topics including Hercules (constellation), NGC objects and Planetary nebulae.

Its subject is documented across 35 Wikipedia language editions.

Key facts

Right ascension
16 44 29.51960
Declination
+23 ° 47 ′ 59.4913 ″
Distance
5.4 ± 1.3 kly (1.7 ± 0.4 kpc ) ly
Apparent dimensions v
40″ × 30″
Constellation
Hercules
Radius
0.5 ly
Designations
PN G043.1+37.7, BD +24° 3048 , HD 151121 , IRAS 16423+2353 , NGC 6210

via Wikipedia infobox

Wikidata facts

Constellation
Hercules
Distance from Earth
2282
Image
NGC 6210 HST.tif
Show 13 more facts
Commons category
NGC 6210
spectral class
Of/[WR]
catalog code
Gaia DR2 1299564195037054592
Commons gallery
NGC 6210
time of discovery or invention
1825-00-00
epoch
J2000.0
apparent magnitude
9.502
right ascension
251.12299832220480
declination
23.79985868534130
radial velocity
-35.6
right ascension component of proper motion
-18
declination component of proper motion
24
Sources (2)

via Wikidata · CC0

~5 min read

Encyclopedic overview

NGC 6210, sometimes also known as the Turtle Nebula or simply the Turtle, is a planetary nebula located approximately 5.4 ± 1.3 kly from the Sun in the constellation of Hercules. It is a bright nebula. It is positioned about 38° above the galactic plane at a vertical distance of about 3.3 kilolight-years (1 kpc), this is unusually high for a nebula. Due to its position, it has little extinction from intervening interstellar dust.

The nebula formed as a result of material being shed from a low mass progenitor star less massive than the Sun (~0.9 M☉) the complex structure and appearance of NGC 6210 has lead to proposals that the nebula was shaped by mass transfer in a triple star system.

Excerpted from Wikipedia’s “NGC 6210” article, available under the CC BY-SA 4.0 licence.

Connections

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