The world is my country, and science is my religion.
/ Christian Huygens /



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.


Show me the newest sketches!
By type: open clusters [67] globular clusters [14] diffuse nebulae [3] dark nebulae [0] planetary nebulae [27] variable stars [18] binary stars [23] asterisms [2] galaxies [119] quasars [1] planets [2] minor planets [1] comets [5] Sun [0] Moon [5] other objects [8]
By catalogue: Messier 1-50 [20] Messier 51-110 [18] NGC 1-1000 [17] NGC 1001-2000 [21] NGC 2001-3000 [32] NGC 3001-4000 [25] NGC 4001-5000 [18] NGC 5001-6000 [22] NGC 6001-7000 [40] NGC 7001-7840 [35] IC 1-5386 [1] other catalogues [71] uncataloged [10] [25]
By constellation:



NGC 3900 (Galaxy)
Right ascension: 11h 50m Declination: 26° 56'
Constellation: Leo
Date/time: 2015.04.09 20:45 UT
Equipment: 12" f/5 Newtonian
FoV: 13' Magnification and filter(s): 250x
Seeing: 7/10 Transparency: 2/5
SQM: 21.02 m/as2 Temperature: 6°C
Humidity: moderate
Sight: 2 - minor details, somewhat interesting
Difficulty: 4 - hardly visible, dark adaptation and very dark skies needed, averted vision is required to see details
Position: 4 - hard, complex starhopping needed
Location: Talpa Minor Observatory
Observer: Ferenc Lovró
Description:

A very faint galaxy, I see no star-like nucleus, however the central regions are somewhat brighter, and show many barely discernible brighter knots on the long axis of the galaxy. High humidity kills details.



This is my first real observation in self-made observatory (besides a quick check of Jupiter without proper collimation after I've transferred my light-bucket to the dome). Climate is excellent, plenty of space, the radio is on, very cozy place. What I've quickly discovered is that I must pay attention not to reach the side of the slit with the OTA's light path plus I've found that the SQM sees quite a lot in infrared despite the block filter in front of its detector. I have a strong infrared floodlight to support my security cameras that are watching the dome, and if I leave the infrared lights on, the SQM measures about 16 MPSAS instead of 21. Sorry for this interruption, now back to the observations. ;)


Hi-resolution image: [ reversed sketch | original sketch ]
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All text and images are ©opyright of Ferenc Lovró. All rights reserved worldwide.

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