Celestial hemisphere:  Southern  ·  Constellation: Dorado (Dor)  ·  Contains:  30 Dor Cluster  ·  40 Sgr)  ·  NGC 1787  ·  NGC 2052  ·  NGC 2070  ·  Part of the constellation Dorado (Dor)  ·  Tarantula Nebula  ·  The star Namalsadirah II (τ Sgr  ·  The star β Dor  ·  The star β Men  ·  The star δ Dor  ·  The star ε Dor  ·  The star η Men  ·  The star η2 Dor  ·  The star θ Dor  ·  The star ν Dor  ·  The star π2 Dor
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Large Magellanic Cloud in Narrowband (OIII-Ha-S2), Bruce Rohrlach
Large Magellanic Cloud in Narrowband (OIII-Ha-S2)
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Large Magellanic Cloud in Narrowband (OIII-Ha-S2)

Getting plate-solving status, please wait...
Large Magellanic Cloud in Narrowband (OIII-Ha-S2), Bruce Rohrlach
Large Magellanic Cloud in Narrowband (OIII-Ha-S2)
Powered byPixInsight

Large Magellanic Cloud in Narrowband (OIII-Ha-S2)

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Description

The Large Magellanic Cloud in a rarely used colour mapping palette of OHS = RGB.

The narrowband data does a wonderful job of accentuating the knotted accumulations of hydrogen, oxygen and sulphur gas that form the flocculent nebula.

This small satellite galaxy in our cosmic backyard has a mass (in different models) of 30-130 billion solar masses, a weight much less than the 1.2-1.9 trillion solar mass estimate for the Milky Way which it orbits.

Recent very high velocity measurements suggest the LMC and the SMC (both satellite galaxies) are making just their first orbit of the Milky Way after being gravitationally captured. However, already there is significant interaction between these 3 neighboring galaxies. The existence of the Magellanic Stream, a tidal tail of gas that has been stripped from the SMC/LMC system and now extends half way around the Milky Way, provides further evidence for interactions between these three galaxies.

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Large Magellanic Cloud in Narrowband (OIII-Ha-S2), Bruce Rohrlach