Maximize your "spacewalk" experience with the 21mm Ethos. Transform your
passage through the Milky Way with the 21mm’s nexus of contrast, power
and field. Larger deep sky objects and rich star fields are its natural
playground. Looking on-axis your field-of-vision is filled with 100º of
stars, however wherever you chose to concentrate your attention you’ll
see sharpness and richer contrast.
The optical performance of the 21mm is the work of Ethos lead designer
Paul Dellechiaie, who achieved a level of optical aberration correction
right in line with his other Ethos designs. Contrast and transmission
have been maximized using the same advanced coating techniques and
further aided by the internal mechanical design techniques used in all
Tele Vue eyepieces.
Extending the Ethos focal length range to 21mm while maintaining the
original performance goals of the rest of the series brings the eyepiece
up against the mechanical limits of the 2” barrel and focus constraints.
The 21mm provides the maximum true field of view, has no significant
vignetting at the edge of the field, and is parfocal with the 31mm Nagler
Type 5.
The 21mm focal length completes the logical set of 21mm/13mm/8mm and
nicely juxtaposes the 17mm/10mm/6mm combination. Each step within these
two sets approaches a 3X field area gain. The 21mm’s effective field stop
diameter is 36.2mm, bringing its true field close to the 35mm Panoptic
(38.7mm Field Stop diameter). Its true field is also larger than the 26mm
Nagler with its 35mm effective field stop diameter. In an f/4 Dobsonian,
the exit pupil is just 5.25mm using the 21mm Ethos instead of 8.75mm with
a 35mm Panoptic, or 6.5mm with a 26mm Nagler.
Like all Tele Vue eyepieces, every 21mm Ethos goes through our optical and cosmetic quality control procedure in Chester, NY and should your eyepiece ever need service we can do everything from replacing a dented barrel to replacing a scratched eyelens.
Since all Ethos models accept Dioptrx, you now also have the “final frontier” – the ability to compensate for your own eyesight astigmatism with a superb multi-coated lens providing your exact correction, rotation orientation and centration over the eyepiece. This is the culmination of our quest to not only bring you observing experiences “…even better than you imagined,” but a 30-year recognition of being “tops in the field.”
Ethos 21mm: First Warranty Card Impressions
Remarkable! The finest piece of equipment I own! This field is stunning and the correction is perfect. A triumph! — BJD, CT
Take my wife, kids, or car, but don't touch my Ethos eyepieces! — BT, ONT
Ethos 10mm: Filling the Gap!
Some Holes Just Need to be Filled!
Ethos 10mm: First Editorial Impression
We got our first peek through Tele Vue's latest Ethos, the 10-mm, and its
performance was truly as incredible as any in that growing family of hyperwide,
supremely-corrected, high-fidelity eyepieces. You'll have to try one in person
to understand the significance of Tele Vue's accomplishment - words cannot
capture the experience.
The 10mm Ethos delivers: 100° apparent field
(50% larger in area than 82° Naglers), comfortable eye-relief, (accepts DIOPTRX
eyesight astigmatism correctors), distortion correction, high contrast and
on-axis sharpness for planetary viewing. It is the “do-it-all” eyepiece perfect
for all scopes that can utilize this focal length. And, "filling the hole"
between the 13mm and 8mm makes it the ideal centerpiece for a 17mm/10mm/6mm
Ethos set.
An important benefit of the combination of large apparent field of view and
shorter focal length is that for a given field in the sky, higher magnification
results in a darker sky background. Fainter stars become visible and more detail
is seen on all deep sky objects. Ethos provides another big
magnification/contrast jump, yielding dramatic views simply not previously
possible in any telescope. With the smaller exit pupil, eyesight limitations are
also reduced.
In
addition to matching all the key performance criteria of its 13mm sibling, its
lighter weight and smaller diameter makes the 10mm more suitable for use with a
binocular viewer.
Celebrate the start of the
International Year of Astronomy 2009, the 400th anniversary of Galileo's
first use of an astronomical telescope, by showing friends and neighbors
the best of our wonderful universe. The Tele Vue philosophy (Ethos, if
you will) has always been about inspiring “spacewalk” vistas by creating
the finest “rich field” refractors and wide angle eyepieces. We hope the
introduction of these new Ethos models will further rekindle the
appreciation of astronomy and support all the worthy goals of IYA 2009.
It’s been quite a challenge to develop new Ethos eyepieces to the same
performance standards achieved by the 13mm and 8mm models, perhaps the
most honored in history. We hope the increased field of the 17mm and
increased power of the 6mm will open up new visual experiences that
Galileo could hardly have imagined, from small refractors to the largest
Dobsonians.
At NEAF 2008 we were pleased to demonstrate a new 8mm focal length,
100° AFOV Ethos eyepiece. In addition to matching all the key
performance criteria of its 13mm sibling, the new 8mm version is
parfocal in 1¼" focusers with Radians, Plössls, Type 6 Naglers and 1¼"
Panoptics. Further, its lighter weight and smaller diameter than the
13mm Ethos makes the 8mm suitable for anyone using a binocular viewer.
Another application is for spotting scope set-ups with the Tele Vue 60°
1¼" diagonal. In comparing it to our 8–24mm Zoom eyepiece, the 8mm Ethos
has the power of the 8mm Zoom and 83% of the field of the 24mm setting!
Ethos principal designer, Paul Dellechiaie, is flanked by Al (left)
and David Nagler (right) for the announcement of the new Ethos 8mm 100°
eyepiece at the NorthEast Astronomy Forum (NEAF) in Suffern, NY, on
April 26, 2008.
Click the image for video playback with audio.
Ethos 13mm - The Tele Vue Ethos Experience
Introduced at Northeast Astronomy Forum
Tele Vue 13mm Ethos™
Tele Vue is known for its in-house eyepiece and telescope designs by Al
Nagler; our latest eyepiece brings new meaning to the term “in-house.” The
concept for this eyepiece was first proposed by Tele Vue President David Nagler,
with performance parameters giving it the fundamental characteristics (the
ethos) of a Tele Vue eyepiece: high contrast, comfortable eye relief and full
field sharpness. Control of astigmatism, field curvature, lateral color, angular
magnification distortion correction (technical reference), and low pupil sensitivity for daytime use
were specified criteria.
Following Tele Vue’s philosophy of pushing the state of the art, long-time
Tele Vue employee and optical design protégé Paul Dellechiaie took up the
challenge and designed the basic eyepiece form. Under Al’s guidance, Paul
tweaked his design to fulfill the original goals.
While sharpness is inherent to the optical design, contrast is maximized
through the intelligent use of flat finished baffles and ultra low reflectance,
high efficiency coatings tuned to the composition of each element.
At the 2007 Northeast Astronomy Forum, Tele Vue once again broadened the
amateur astronomer's
perspective on the universe and introduced a new observing experience;
100º of pure Tele Vue quality. With a 13mm focal length evoking the original
“Nagler” revolution, the field area of this new eyepiece is more than 50% larger
than an 82º field. The Tele Vue Ethos is essentially multiple eyepieces,
delivering the true field size of a longer focal length, narrower apparent field
eyepiece with the benefits of higher power and darker sky background.
We invited NEAF attendees to take a look and see the universe the way we
think it was meant to be
experienced, with a field of view incredibly wide and sharp! We were very
pleased indeed by the response and validation of our design goals.
At Tele Vue, we prefer not to have recommendations with asterisks. For this reason,
we have not specifically endorsed the 13mm Ethos for Bino-Vue use because of the
63.5-mm diameter barrel (=63.5-mm interpupilary distance). Even so, we were
advised by Mike Harvey at the Winter Star Party (2008) that only 1-person in 25
had interpupilary limits with the bino'd Ethos.
However, since many of our customers have been thrilled with the experience,
we have maximized the potential use by narrowing the barrel from 63.5-mm to
62-mm diameter for eyepieces delivered beginning mid-March 2008. While the
difference is only 1.5-mm, (or 0.75-mm for pairing a first production unit with
current production) we decided to make this small change public, in case you
want to give it a try.
Following are some of Mike Harvey’s Winter Star Party Ethos experience
comments posted on Cloudy Nights’ Eyepiece Forum.
13mm ETHOS' in a binoviewer!
Excerpts fom Mike Harvey's posting on CloudyNights.com, Feb. 10, 2008
WOW! OMG! (and many "expletives deleted"!).
Forget about the 100-degree field (well...I know you can't but...), this is
quite simply the finest eyepiece I've ever seen - period! Contrast, sharpness,
light-throughput, etc. are all just amazing. There is simply NO ghosting or
other internal reflections...the background is jet-black and the stars (even in
my 28" f/3.66) are absolute diamond-points to the very edge!
I've owned and used all of the "gold standards" over the years and NOTHING
I've seen can match this!
Along with about a half-dozen other observers we did "A/B" testing with other
top-of-the-line 13 and 14mm eyepieces (M-51, Thor's Helmet and M-42 were the
targets). EVERYONE agreed that the ETHOS seemed to add additional inches of
aperture. The increased detail in all of the objects was instantly apparent!
As a bonus, the fine detail on Saturn equaled or exceeded the best
"planetary" eyepieces any of us had ever used. And, again, NO ghosting or
internal reflections. This baby does it all.
And, as for the 100 degree field, Vic said it best... "you feel like you're
going to fall in"..."the scope just gets out of the way and it's like you're
standing in space looking at the objects".
If I were only going to have ONE eyepiece (or one 'pair') THIS IS IT!
Bright crisp clean sensation, very forgiving on f/5 optics, and that FOV. Oh,
that field! Masterpiece. Thank you very much. — B.D., CT
High quality, state of the art. Continuous FOV without distortion. Affordable.
— G.M., CA
Wow!!!!! Great, nothing better. — J.W., CA
Tele Vue has once again completely re-defined the eyepiece, setting an even
higher standard by which all others will be judged. The Ethos exceeds my wildest
dreams & imagination! — D.G., TX
The Grand Canyon of eyepieces! — R.B, CT
Pin points everywhere — P.T, QU
It has the "You are there" experience on all my telescopes — K.B, ON
Fantastic! — D.B, MI
Outstanding! — C.C, MO
Wonderful — E.C, PA
A railing should be mounted around the Ethos in order not to "fall into the universe" ;-) — S.S, Germany
It's the best! — M.B, CA
Excellent contrast and the field of view is something else, even compared to Naglers. — J.R, CA
Very satisfied and can find DSOs easier. Objects look superb in quality. — M.M, CA
Impressive! To say the least. — P.W, SC
Absolutely amazing contrast. This eyepiece takes visual observing to the next dimension. — G.S, ON
Jaw dropping when just slewing across the zenith. — F.L, PA
Sensational! — N.P, Australia
Ethos - Best eyepiece made. — D.D, IL
I'm speechless. — B.N, CA
Breathtaking! Congratulations! — Z.N, Austrailia
Amazing! — J.K, BC
Impressive -- especially in small refractors, lots of stars-sharp to the edge. — P.S, England
Ethos™: The "Majesty Factor"
The Nexus of Contrast, Power, Field
— an essay by Al Nagler
"Majesty Factor" Summary
To illustrate the dramatic effect of combining a larger apparent field
(yielding greater deep sky details) with smaller exit pupils (yielding fainter
stars with darker sky background) we propose the "Majesty Factor". We define it
simply as the cube of the ratio of any two different apparent field eyepieces
having the same field stop diameters (same true field). Examples:
(100°/70°)3 = 2.92
"M.F." or (70°/50°)3 =
2.74 "M.F." or (100°/50°)3
= 8 "M.F."
After showing Ethos at a number of events since April 2007, we can safely
conclude it brings the observing experience to a new level. This is based solely on
user's reactions to views of familiar objects, not on any prejudgments,
publicity or hype on our part. While we were quite confident of success,
we wanted, and still want, to explore all the ramifications of what a sharp 100°
field really represents.
Right after NEAF in April, Rodger Gordon, the acknowledged "eyepiece junkie" of
all time, wrote me "Definitely the finest wide-angle eyepiece I've ever seen. If
God is an astronomer, this is the wide-angle eyepiece he'd choose. You can quote
me." Thanks, Rodger. I waited until now to avoid "priming the pump", so to speak
before quoting your unbridled enthusiasm publicly.
For some time, I've been pondering just why the response has been so
overwhelmingly positive. And if I really understand why, is it possible to
quantify? My views of the Double Cluster at Stellafane pointed the way.
The 1991 article I wrote for Sky and Telescope on magnification
provides the key. A major conclusion for low power states: "The best view occurs
with the highest power that comfortably includes the target object. Higher
powers darken the background sky, reveal fainter stars and show more detail.
The resulting smaller exit pupil also minimizes the effects of eyesight
defects."
Considering the potential of Ethos, let me posit a more general conclusion:
For deep sky viewing of star fields, open and
globular clusters, nebulae and galaxies, choose the highest power that frames
the subject, so long as the sky background does not reach black, and the
atmosphere does not degrade the resolution. The smaller exit pupils permit
a darker sky background which achieves greater contrast against the fixed
brightness of stars, while the greater magnification reveals more structural
details on extended objects. Using eyepieces with larger apparent
fields maximizes the viewing experience.
The result is an increase in what I would call theMajesty Factor, the nexus of
contrast, power and field.
It's clear that the largest possible apparent field for a given true field
yields the most magnification for greater resolution, with a darker sky background
for more contrast as a result of the smaller exit pupil. I believe this combination
of contrast, power and field causes the typical "wow" reaction
— the Majesty Factor. I think Tom Trusock
said it most succinctly in his Starfest (Canada) report: "The same true field at
higher magnification means that you'll see blacker skies and more detail."
Dennis di Cicco in his 5-star review of Ethos in his October 2007 Sky & Telescope
review
noted something similar: "Observing with the 12-inch scope, I typically bounce
between a wide-field eyepiece for star-hopping and a high-power one for
detailed views. But the Ethos gave me both. The field was large enough to
star-hop, and the magnification was high enough to bring out faint stars and
resolve details in galaxies and star clusters." (He coincidently also
illustrated field sizes using the Double Cluster.)
Let's try to quantify the so-called Majesty Factor. While we cannot quantify the majesty of a great
symphony, work of art or edifice, I think a meaningful Majesty Factor is
quantifiable for those great deep sky views. Here's how:
For Reference
Basic Telescope and Eyepiece Concepts
apparent field: perceived span of sky seen through eyepiece
(without telescope). Not used in true field (see) calculation.
exit pupil: image of objective formed by eyepiece. Location
where full apparent field is seen.
f/#: a ratio that describes the relation between the aperture
and focal length of the telescope -- important for photography
field stop: ring inside the eyepiece barrel that limits true
and apparent field size
focal length: effective distance from entrance of an optical
system to focal point
magnification: relative change in angular size of object
true field: span of sky seen through telescope/eyepiece
combination
Basic Telescope and Eyepiece Formulas
Let's consider a range of possible eyepieces with apparent fields of 50°,
60°, 68°, 82° and 100°. Now let's pick an object, (like the Double Cluster) and let's say it's properly framed in the field of a 50° Plössl with a 26-mm
focal length in an f/4 telescope so the exit pupil = 6.5-mm. Let's
arbitrarily assign a factor of 1 to the power (magnification) of this telescope
and a factor of 1 to represent the contrast for the 6.5-mm exit pupil.
Therefore, for the given true field, the
Majesty Factor = 1 (power factor) x 1 (contrast factor) = 1.
Now let's replace
the Plössl with a 100° (apparent field) Ethos with a 13-mm focal length. This
yields the same true field of view at twice the power with twice the
apparent field and half the
exit pupil. The 3.2-mm exit pupil is only ¼ the
area of 6.5-mm, so the sky background darkens by a factor of 4 (contrast factor).
The magnification power factor yields twice the detail or resolution. Therefore:
2 (power factor) x 4 (contrast factor) = 8x
Majesty Factor
Working out the math for all the apparent fields listed above, we have:
Majesty Factor for Various Apparent Fields
for Eyepieces Yielding Same True Field
Apparent Field (°)
Power Factor
Contrast Factor
Majesty Factor
Plössl
50
1.00
x
1.00
=
1.00
Radian
60
1.20
x
1.44
=
1.73
Panoptic
68
1.36
x
1.85
=
2.52
Nagler
82
1.64
x
2.69
=
4.41
Ethos
100
2.00
x
4.00
=
8.00
A simple rule of thumb is that for any two eyepieces having the same true
field of view, the Majesty Factor equals the cube of their apparent field
ratios. Example is (100°/70°)3=2.92.
— Al Nagler
TV60is image of Double Cluster by Robert Reeves
Majesty Factor Visualization: 13-mm Ethos (left) and 26-mm Plössl (right) have
same true field of the Double Cluster. But Ethos has twice the power factor
and four times the contrast factor. Ethos therefore has a Majesty Factor of eight
relative to the Plössl's Majesty Factor of one. For reference, the 0.9°
true
field shown could be produced by a 14" f/4 telescope using the 100° Ethos at
109x with a 3.2mm exit pupil or the 26-mm 50° Plössl at 55x with a 6.5mm exit
pupil.
Field Report on Ethos™
— by Al Nagler
The Ethos has now been shown at NEAF, TSP, RTMC, and EPOCH 2007. We thought
you’d enjoy sharing in the experience by reading some of the comments written
in our “comment” notebook. The following display was created for daytime
observation using the Ethos in an NP127is at NEAF and TSP, and an NP101 at
RTMC.
The left chart has circles representing field diameters of 50°, 60°, 68°, 82°
and 100° with the telescope distance set so that the 100° circle matched the
view of the Ethos field-stop. The “crosshairs” are actually small Saturn
drawings in 5° increments to illustrate the linear angular-magnification
correction. Illustrations of Saturn were placed at the center and edge of the
field so contrast and detail (including newsprint dot patterns) could be
evaluated.
The chart to the right is an artificial very-rich “star field” made (and
conceived) by Rick Scheck in our scope production dept. The bright “star”
reflections made a more realistic contrast simulation than simply viewing
astronomical pictures and helped to give a “night sky” impression that nicely
represented a dense Milky Way star field.
Real night-sky viewing was done two nights at the dark Prude Ranch location of
the Texas Star Party using telescopes ranging from our NP127is to the prize
winning 12” f/5.5 Newtonian of our own Scott Ewart. Ethos also made its way
into various large Dobsonians including those of Barbara Wilson and Larry
Mitchell.
At the Riverside Telescope Makers Convention in California, we had two clear,
though very bright moonlit nights for evaluation. Using an NP101 and NP127is
Ethos treated us to clusters such as M44 and M24.
At EPOCH 2007 in western Indiana, we were pleased to have one very clear
evening to demonstrate Ethos with our NP127is and Chris Brownewell's 25"
Obsession. Good Luck, Chris, on this new star party venture, and a big Thanx
for being a great host.
While all of us at Tele Vue are proud and excited by the response, it’s much
more interesting for you to note the recorded comments. On a personal note, I
was especially moved by just showing a random star field to a little
10-year-old girl in a group visiting RTMC from Anaheim. Her only words: “Oh my
god, it’s beautiful.” It doesn’t get any better than that.
— Al Nagler
Kudos to our Paul Dellechiaie, the principal designer of Ethos.
ETHOS Comments
NEAF 2007 Comments
Wow! What a view! Clear right to the very edge. - C.M.
Absolutely the best wide angle eyepiece I’ve ever seen - the 100° FOV. - R.W.G.
The star field was “a religious experience”! - M.S.M.
Another winner. Unbelievably wide. - S.F.
It’s so good it’s scary. - R.F.
Space-walk plus. - D.S.
TSP 2007 Comments
Incredible field - sharp. - L.G.
Sharp as a tack from edge-to-edge. - J.E.
Extraordinary field-of-view. - R.J.
Amazing! Very usable field - better than I imagined it could be! - T.B.
Enchanting. - J.H.
I could see no edge distortion to the edge of the field anywhere. Very nice
contrast. - M.P.
Just need to add the helmet for the full spacewalk experience! - T.W.
Totally immersive experience! Thanks for bringing products like this for us
astronomers! - D.A.
Terrific experience!! - J.C.
Very impressive. - M.S.
Wonderful!!! - C.C.
Remarkable. - R.M.
Great! The Ethos sets the bar even higher; advances the hobby yet again. Super!
- A.D.
Outstanding - can’t wait. - D.M.
Oh my God that’s incredible. - J.R.
Excellent additional real estate in the wide field of view. - D.C.
Thanks for making astounding equipment! - T.K.
Awesome view through the Ethos! - K.P.
The 13mm Ethos is an eyepiece that you can get lost in. You feel as if you
could almost look behind you. - R.T.
Ethos is super and can’t wait! Thanks, you and Tele Vue are the best! - A.A.
Really do appreciate the view. - B.A.
Nice, keep it lightweight. - K.M.
Excellent - beautiful under the stars in the refractor! Great with my 20” f/4
on the Coma Cluster and the heart of the Virgo Cluster - makes my wide field
f/4 better at wide fields! - B.W.
Awesome view! - R.C.
Great. - M.F.
Very impressive 13mm on 127. Can I buy the star field!! - J.R.
Ethos eyepiece does impress and another example of Tele Vue excellence. - L.D.
The new eyepiece is a very easy eyepiece to see from. Has good eye relief, and
is very clear. Everyone should have one. - J.D.
Amazing! Sharp to edge. Virtually a binoc view. - J.B.
Incredible sharpness edge-to-edge! - R.L.
Amazing eyepiece! M13 (wow). - J.L.
Oh WOW! - J.P.
Nice eyepiece. - J.A.
You can almost see behind you, wonderful. - D.R.
RTMC 2007 Comments
WOW you did it again. I like it. - D.D.
WOW! Tele Vue Visionary at its best! - T.P.
Wow dizzy. - P.B.
Wow it’s so wide it’s hard to find the edge. - C.E.
Aghaaa 100° a galactic experience. - E.M.
Can’t believe the view. - M.C.
That’s incredible! - E.E.
Impressive!! - F.J.E.
Very nice to edge. - T.C.S.
The most perfect wide-field optics EVER! Wow! - G.C.
Oh my goodness! - K.K.
Once again Amazing! I want one! - G.
Love at 1st light. Very nice. Keep it up. - G.S.
Wow! That’s amazing!
Killer!!! I Need one! - R.L.
What a view! - L.K.
Rather amazing! - J.M.
That’s a great view, sharp all the way across!
Incredible. - R.G.
Goodness Gracious. - T.D.
Very good, very good, I love it. - M.
Great! - J.S.
Fantastic wide field. I almost have to imagine the field stop! And can’t wait
to try one in both my TV-140’s.! - E.S.
When you look thru this piece be careful not to fall onto the view?!
Breathtaking. - S.S.
It’s amazing. - J.L.
It’s like a porthole to space. - G.N.
After reading reviews waiting to get a close-up look I was blown away with the
eyepiece. Sign me up I want one!! I was inside the telescope reaching out to
touch the stars. Amazing!!! - G.W.
100° WOW I love it! - S.A.
EPOCH 2007 Comments
Large Field! Wow! Great to have the magnification and the wide field. Best of
both worlds. Eyegasm! - Chip (16" Lightbridge)
Be prepared to look around! The Ethos was lighter than I thought it might be
and there was no coma at all in my 20" f/5 Obsession. M-27 was fantastic as was
M-13. Viewing the double-cluster thru a TEC 6" I felt like I needed someone to
hold onto the back of my shirt so I wouldn't fall in! It's on my list to get!
Thanks for the views Al. -- M.M.
Fantastic - wow - a real winner! Very undistorted. Thanks Al. -- F.H.
Spectacular! Beautiful eyepiece, very comfortable to look through. Thank you
for bringing Tele Vue to Indiana. -- A.M.
Super Wide Field - Excellent. -- anon.
13mm Ethos - Awesome F.O.V.! Almost too much to take in at once. Can't wait to
get one! -- D.H.
Wow! Wow! -- J.M.
Sweet! Great View. -- R.M.
Once again - as usual
- we can offer perfection to our discriminating customers -- thanks to Al
Nagler for making it fun to be a telescope dealer. -- W.M.
Just didn't think a "31" could be one-upped. I was wrong!! Incredible!! --
anon.
Super Wide Field Ethos eyepiece: Lagoon nebula had clarity of stars
edge-to-edge in view. All stars "tack" sharp. M13 was as if I'd never seen it
before. Outstanding. -- J.M.
Super wide field - unbelievably exceptional / outstanding view; crisp, clear --
wow!! Don't think I've seen anything that great until now. -- S.
The field-of-view is so extensive that I had to almost crawl inside to look at
it all. -- C.D.
Looking through Ethos 13mm gave me the same exciting feeling I got looking
through a Nagler the first time. Same WOW factor. Can't wait for high power
Ethos. -- B.C.
Stellafane 2007 Comments courtesy Dave Mitsky
The two most memorable sights of the night for me were both through Tele
Vue's incredible 100 degree AFOV 13mm Ethos ocular. M27 through John Vogt's
32" ATM Dob and the Ethos was truly unbelievable and I've never before seen
M31 as mind-blowingly extended as I did through Al Nagler's 127mm Tele Vue
apochromat and the Ethos. This yet-to-be released new eyepiece is simply
amazing. -- Dave Mitsky, A Brief Report from Stellafane 2007,
bautforum.com
Starfest (Canada) 2007 Comments courtesy Tom Trusock
[B]lew me out of the water. We used it on the NP101 and a 20" f5 obsession
- to spectacular results with both. This eyepiece takes the Nagler philosophy
to the next level - The same true field at higher magnification means that
you'll see blacker skies and more detail. So, although it's extremely
impressive, the massive sense of immersion could almost be considered a
secondary effect.
But what a secondary effect.
For me, the most striking view this weekend was of M31/32/110 in the NP101
- simply amazing. On this scope, the eyepiece generates about 40x, and nearly
a 2 and 1/2 degree field! It was really funny to see a line of up to 20 people
in front of this little 4" telescope, and the huge 20" f5 right next to it
sitting totally empty. This was definitely one night where aperture didn't
win.
The Ethos is truly the next revolution in visual astronomy.
-- Tom Trusock, First Light - Ethos, cloudynights.com - eyepiece forum
Eyepiece Distortion
Technical Reference: Telescope Optics by Rutten & Van Venrooij, page 169
“Distortion becomes especially
important in wide-field eyepieces. In discussing distortion, however, one must
clearly distinguish between rectilinear distortion and angular magnification
distortion. For terrestrial telescopes, it is often required that straight
lines in the focal surface look straight in the eyepiece. For zero rectilinear
distortion, the following relationship should apply:
y =
f ∙ tan ß
where y is the
off-axis distance in the focal plane, ß the image angle from the optical
axis, and f the focal length of the eyepiece.
For astronomical observation,
however, it is important that the angular magnification remains constant over
the field. For instance, the angular distance between double stars should be
the same and a round object (a planet) should retain its shape whether viewed in
the center of the field or at the edge of the field. In this case, the
following relationship should apply:
y =
f ∙ ß
where ß is expressed in radians.
With zero angular magnification
distortion, straight lines on a focal plane appear curved in a pincushion
fashion, with the curvature becoming greater the farther they lie from the
center. It is impossible to correct an eyepiece simultaneously for rectilinear
and angular magnification distortion.”
Al Nagler notes:
For reference, the maximum angular magnification
distortion of the new 13mm Ethos is no more than 1% at any point in the 100˚
field