Constellation: Ursa Major
Right Ascension: 09h 47m 30.71
Declination: +63° 14` 53.3
Distance: 246 ly
Apparent Magnitude: 6.94
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HD 84406 is located in the constellation of Ursa Major, and a yellow star of spectral type G, and shines at a magnitude of 6.9, just dimmer than a person can see without optical aid.

What is special about HD 84406? Actually not too much as stars go, but that is a good thing as it was used for the initial focusing of the new James Webb space telescope.

Some of the constraints were the star would have to be in the field of view for the telescope for the entire collimation of the mirrors. The star couldn't be too bright which would cause issues with the sensors. Also the star needed to be in an uncrowded area by other stars. And of course the star needs to be stable with a constant magnitude.

Telescope: GSO RC10
Camera: ZWO 2600 MM
Constellation: Leo
Right Ascension: 10h 56m 28.99s
Declination: +07° 00′ 52.0″
Distance: 7.9 ly
Apparent Magnitude: 13.5
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A red dwarf star located in the constellation of Leo, its the reddish star located in the center of the image. It's name comes from astronomer Max Wolf who studied that exhibit large proper motion across the sky. A star with a large proper motion appears to move across the sky over the years. Most are relative close stars that their movement can be measured over the years.

One of the closer stars at 7.9 light years, but because its one of the dimmest of the local red dwarfs, its magnitude is a faint 13.5.

Image of Wolf 359 taken in 2015, compared to its current location shows its movement over the years.

Telescope: GSO RC10
Camera: ZWO 2600 MM
Constellation: Canis Major
Right Ascension: 07h 22m 58.32877s
Declination: −25° 46′ 03.2355″
Distance: 3,820 lly
Apparent Magnitude: 6.5–9.6
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VY Canis Majoris is a hyper giant star, one of the larger known stars. If this star was placed where our Sun was, it would extend out past Jupiter. The star is loosing mass due to its low surface gravity and extreme stellar wind, and is surrounded by a envelope caused by the mass loss. Due to its extreme size and mass, for a star, it will have a short lifetime and probably will go supernova within 100,000 years.

Annotated image follows.

Telescope: GSO RC10
Camera: ZWO 2600 MM
Constellation: Perseus
Right Ascension: 04 29 18.85
Declination: +43 54 23.0
Apparent Magnitude: 8.5 - 15
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Discovered Nov 25, 2020, this time-lapse of Nova Per 2020 covering the period of Dec 8 - Mar 18. Images were taken about every two weeks weather permitting. Started with a brightness of mag 9, fading to mag 15.

 

Telescope: Explore Scientific 127 Refractor
Camera: ZWO 1600 MM
Constellation: Sagittarius
Right Ascension: 17h58m16.1s
Declination: -29°14'57"
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Quick capture of Nova Sgr 2021 No.2 (V6595 Sgr) from last night. Discovered on April 4th, currently around Mag 8.

Telescope: Explore Scientific 127 Refractor
Camera: ZWO 1600 MM
Constellation: Corona Borealis
Right Ascension: 15h 49m 31.31093s
Declination: +39° 34′ 17.9111″
Distance: 8815 ly
Apparent Magnitude: 7.8 - 10
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V Crb is a red giant Mira type carbon star located in Corona Borealis. 

Telescope: Explore Scientific 127 Refractor
Camera: ZWO 1600 MM