We owe our existence to stars, because they make the atoms of which we are formed. So if you are romantic you can say we are literally starstuff. If you're less romantic you can say we're the nuclear waste from the fuel that makes stars shine.
/ Sir Martin Rees /



In memoriam Halton C. Arp (1927-2013).


My astronomy sketches. Hover mouse over image for the inverted look. For fainter objects, take a look at the black-on-white original, sometimes it reveals more details.


Need advice? Want to discuss an observation? Feel free to contact me at flovro gmail*com.

ÚJ! Amennyiben elérhető, a ikonra kattintva magyarul is olvashatod az észlelést.


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NGC 7052 (Galaxy)
Right ascension: 21h 19m Declination: 26° 31'
Constellation: Vulpecula
Date/time: 2016.08.03 22:30 UT
Equipment: 12" f/5 Newtonian
FoV: ' Magnification and filter(s): 250x + 15 filter(s)
Seeing: 8/10 Transparency: 5/5
SQM: 21.48 m/as2 Temperature: 17°C
Wind: none
Sight: 2 - minor details, somewhat interesting
Difficulty: 3 - moderately visible, dark adaptation needed, averted vision might add to details
Position: 3 - moderate, some starhopping needed
Location: Talpa Minor Observatory
Observer: Ferenc Lovró
Description:

Elongated to the WSW-ENE direction, this is a surprisingly small galaxy - at least I've expected a much larger object based on my map. Its surface brightness is however way higher than expected. It's core is not visibly brighter than the rest, but its WSW side is a bit brighter and this side of the galaxy is also better defined, the ENE side disappears in the sky background gradually. Is this phenomena perhaps a result of a spiral structure?To the East of the core, outside of its body, a tiny (foreground) star is very apparent.


Hi-resolution image: [ reversed sketch | original sketch ]
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