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poppasmurf

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poppasmurf last won the day on February 8

poppasmurf had the most liked content!

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About poppasmurf

  • Rank
    Termination Shock
  • Birthday 03/21/1966

core_pfieldgroups_99

  • Biography
    only actively involved in am astronomy since 2007.
  • Location
    Wangaratta,Victoria, Australia
  • Occupation
    Projectionist
  • Astronomy Equipment
    8" GSO RC
    Moonlite CS focuser
    Skywatcher NEQ6PRO
    Meade DSI
    Imaging Source DBK21AU618.AS
    tasco galaxsee 114500
    Televue powermate 5X
    fujifilm s96

Profile Information

  • Gender
    Male
  • Location
    Wangaratta, Victoria, Australia
  1. Pearl Cluster

    Data captured between 27/04 & 03/05, 4 hrs total. Object:NGC 3766 Object Info: NGC 3766 is an open star cluster in the southern constellation Centaurus. It is located in the vast star-forming region known as the Carina molecular cloud, and was discovered by Nicolas Louis de Lacaille during his astrometric survey in 1751–1752. At a distance of about 1745 pc, the cluster subtends a diameter of about 12 minutes of arc. There are 137 listed stars, but many are likely non-members, with only 36 having accurate photometric data. Total apparent magnitude of 5.3 and integrated spectral type of B1.7. NGC 3766 is relatively young that is estimated as log (7.160) or 14.4 million years, and approaching us at 14.8 km/s. This cluster contains eleven Be stars, two red supergiants and four Ap stars. 36 examples of an unusual type of variable star were discovered in the cluster. These fast-rotating pulsating B-type stars vary by only a few hundredths of a magnitude with periods less than half a day. They are main sequence stars, hotter than δ Scuti variables and cooler than slowly pulsating B stars. Number of Subs: L 60 , R 60 , G 60 , B 60 Sub Length: 60 sec Total Integration Time: 4 Hrs Date Captured: 27/04/2020 & 03/05/2020 Imaging Camera: Moravian G2 2000 Imaging Telescope: GSO RC8 CF Reducer: no Focal Length: 1625 Image Scale: 0.94 arcsec/pixel Field of View: 19 x 25 arcmin Mount: Ioptron CEM60 Guide Scope: Orion ST80 Guide Camera: Prostar LP colour (toupcam) Capture Software: Voyager Guide Software: PHD Guiding 2 Processing Software: PixInsight Shane
  2. My Current gear April 2020

    GPS is amazing. My Ioptron CEM60 has a built in gps unit. Shane
  3. My Current gear April 2020

    Hoping to get some data on the pearl cluster tonight. Shane
  4. My Current gear April 2020

    Yep love multiple monitors. I plan on adding 1 more to my obs (currently 2) which will work perfectly for me with the software I run. No pics of my obs warm room untill I clean it up a bit . Shane
  5. Arp214 (NGC3718) and friends

    Nice work mate. Do you plan on grabbing more frames to clean it up? Shane
  6. A decade of astrophotography

    Wow. Awesome. Shane
  7. NGC 3201

    Well out of practice with both capture and processing but better than the last few months of nothing. Object:NGC 3201 Object Info: NGC 3201 (also known as Caldwell 79) is a low galactic latitude globular cluster in the southern constellation of Vela. It has a very low central concentration of stars. This cluster was discovered by James Dunlop on May 28, 1826 and listed it in his 1827 catalogue. He described it as "a pretty large pretty bright round nebula, 4′ or 5′ diameter, very gradually condensed towards the centre, easily resolved into stars; the figure is rather irregular, and the stars are considerably scattered on the south". The radial velocity of this cluster is unusually high at 490 km/s, larger than any other cluster known. This corresponds to a peculiar velocity of 240 km/s. While high, this is lower than the escape velocity of the Milky Way galaxy.[10] It is located at a distance of 16,300 light years from the Sun and has an estimated 254,000 times the mass of the Sun. This cluster is about 10.24 billion years old. The stellar population of this cluster is inhomogeneous, varying with distance from the core. The effective temperature of the stars shows an increase with greater distance, with the redder and cooler stars tending to be located closer to the core. As of 2010, is one of only two clusters (including Messier 4) that shows a definite inhomogeneous population. Number of Subs: L 50 , R 50 , G 50 , B 50 Sub Length: 30sec Total Integration Time: 120min Date Captured: 04/02/2020 Imaging Camera: Moravian G2 2000 Imaging Telescope: GSO RC8 CF Reducer: no Focal Length: 1625 Image Scale: 0.94 arcsec/pixel Field of View: 19 x 25 arcmin Mount: Ioptron CEM60 Guide Scope: Orion ST80 Guide Camera: Prostar LP colour (toupcam) Capture Software: Voyager Guide Software: PHD Guiding 2 Processing Software: PixInsight Shane
  8. Dark Matter

    Well as I always say Greg, you can’t let the truth get in the way of a good story. Shane
  9. Hyperstar III/C11 running again

    You’re not wrong Tim. I upgraded my old neq6 roughly 6 months ago. I love the new cem60 but life and mostly weather, both natural and fire related, have been a pain and I have hardly opened the obs in the last 6 months. Shane
  10. Christmas 2019

    It's no different over here in the East gents, been bloody aweful the last few months. Shane
  11. Christmas 2019

    right back at ya Dave and the few who still frequent here
  12. Crikey..!!!

    Ripper pics Daryl, the wife and I were over Horsham way just last week. Although we spent most of our time in/around Halls Gap. Beautiful part of the world. Shane
  13. Ribblehead Viaduct Nightscapes

    nice Gordon Shane
  14. Observatory Rebuild

    Looks like cement sheet to me Tim. Shane
  15. Observatory Rebuild

    looking good buddy. Shane
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