Jump to content

Leaderboard


Popular Content

Showing most liked content since 01/19/2020 in all areas

  1. 2 points
    Glad you got it sorted out Greg. My own CGE Pro mount is currently only good for manually choosing targets. I guess if I was old school, I would learn to use those R/A and declination guides. Nah, I'm a wuss. A new mount will be in order soon. Should have a lottery for these bloody things as much as they cost Tim.
  2. 1 point
    No Comment. Just to let y'all know I am still alive Dave VID-20191223-WA0000.mp4
  3. 1 point
    I haven't used the Hyperstar in around a year, so when I checked on it last week - it wasn't working of course. However a week of working on the computer and upgrading the handset (it didn't know what 2020 was before the upgrade) and it is now once again in full working order. Managed a few subs last night between banks of cloud and all looks fine. Looking forward to some deeeep Hyperstar images next clear Moonless night. Greg
  4. 1 point
    Interesting! One of the issues sorted on the Hyperstar III was a dead video card as well!! Greg
  5. 1 point
    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
  6. 1 point
    Your collection on FB speaks volumes mate. You are doing great work. This glob is awesome, and globs come with their own set of challenges. Ray
  7. 1 point
    2019 was the worst year for imaging for me since I started in Autumn 2004 - and it is continuing into 2020. We have complete cloud cover and rain every day. Greg
  8. 1 point
    Well as I always say Greg, you can’t let the truth get in the way of a good story. Shane
  9. 1 point
    Be interesting to see how this plays out. Political correctness, isn't always; correct. Tim.
  10. 1 point
    Prof I will PM you. Ray
  11. 1 point
    I had a PM from a member on Ancestry. At first I thought it was some type of scam, but there was a DNA alert flashing on my account saying something like "father, exact match" or something similar. So it was pretty cool. We made contact and sure enough, a whole new family. Crazy. Ray
×