Messier 54

Observation Notes:

This is the most eastern of 3 globular clusters I observed at the base of the Sagittaruis teapot on 10/3/04. The others were M69 and M70, and M54 was brighter than both of those, with a sharper, more condensed nucleus. I couldn't resolve any stars, even with the 10 mm eyepiece (120X). After some time spent observing, it seemed like I could see a single starlike point to the N of center. But not sure. It might have been a foreground star, or your basic eyestrain illusion.


While M54 is a visual neighbor to globular clusters M69 and M70, recent findings indicate that is probably not a member of our galaxy at all, but a member of the newly discovered Sagittarius Dwarf Elliptical Galaxy. This would put M54's distance at 87,000 light years--nearly 3 times farther out than M69 and M70--making it one of the most luminous globular clusters known with a luminosity of 850,000 suns. At that distance, its diameter would be an immense 300 light years. It is moving away from us at 142 km/sec. Because of its great distance, even large amature scopes cannot resolve it into individual stars, although it can give a mottled appearance from knots of stars within the cluster. These can appear stellar, so that might explain the one starlike point I noticed.

SubjectM54/NGC 6715
ClassificationGlobular Cluster
PositionSagittarius [RA: 18:55.1 / Dec: -30:29]*
Date/Time10/3/04 - 9:00 PM
Observing Loc.Flagstaff, AZ - Home
InstrumentOrion SVP 6LT Reflector (150 mm dia./1200 mm F/L)
Eyepieces/Mag.32 mm (37X); 10 mm (120X)
TransparencyMag 4.5

* Based on published data.

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This page contains a single entry by Jeremy Perez published on October 3, 2004 9:00 PM.

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