I have to admit I don’t fully grasp Barlow functionality.
I believe the distance from the eyepiece to the Barlow lens at the bottom of the barrel can affect how much magnification that combination produces. That potentially, a 2x Barlow might actually be a 1.9x or 2.1x depending on what eyepiece is inserted.
Of course I could be all wet too.
Anyway, I want to find a good Barlow, ie, sharp optics, no vignetting, and a true 2x magnification.
I am considering the TV 1.25” Barlow, assuming it scores on the first two concerns, but am not sure of the true 2x. Especially using non-TV eyepieces.
If not that one, a better recommendation?
Any guidance?
Sam
TeleVue eyepieces in 1.25" have their focal planes about 0.25" below the shoulder.
A TeleVue 2X Barlow is 2.0x with a TeleVue 1.25" eyepiece with that focal plane position.
So if the focal plane of your eyepiece is at the shoulder, the 2X Barlow will be a bit more than 2.0x, maybe 2.05x or 2.1x.
I don't have the focal length for this Barlow, so I cannot tell you what it will be, but the chart on the TeleVue site:
https://www.televue....d=52&Tab=_photo
implies the magnification increase is about 0.014x per mm of distance.
That would mean an increase of 0.09x at the opening of the Barlow = 2.09x. TeleVue's chart can be read as 2.1x at that level, so, rounded off, 2.1x at the shoulder, and 2.0 times 6.35mm into the tube.
I suspect you will have similar findings on most Barlows, i.e. that they are not exactly as claimed at the opening of the Barlow.
And if your eyepiece has its focal plane at a location other than the shoulder, the odds are not high the Barlow will be exactly as claimed.
You don't have to read many Barlow threads here on CN before you realize that the magnification of most Barlows is +/- from the rated power.
Exceptions would include the 2x, 2.5x, 4x PowerMates:
https://www.televue....?id=53&Tab=_app
which change only minutely with small changes in eyepiece focal plane positions.
One way to gauge the exact magnification of a Barlow requires a field test:
Time 1: time the passage of any star across the field from edge to edge through the center
Time 2: add barlow and repeat the timing on the same star.
Time 1 ÷ Time 2 = magnification factor.
Here is info on the Baader VIP Barlow:
https://www.baader-p..._vip_barlow.pdf