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13mm Ethos

$620.00
[ETH-13.0]
In Stock
Tele Vue 13mm Ethos Specifications

Apparent Field: 100º
Focal Length: 13mm
Effective Field Stop: 22.3mm
Eye Relief: 15mm (accepts DIOPTRX™ eyesight astigmatism corrector)
Barrel Size: 2" & 1¼"
Weight: 1.20 lbs. / 19.2 oz.


One of the five original 13mm Ethos eyepieces
at the Rocky Mountain Star Stare





Excerpts from Sky & Telescope, October 2007, review by senior editor Dennis di Cicco
A Triple-Digit Field of View
Tele Vue’s new 13-mm eyepiece is about to transform deep-sky observing.

S&T RATINGS
Optical Performance
Sensibly perfect. No meaningful improvements possible.

Just as the original 13-mm Nagler set a new standard for deep-sky observing in 1981, the Ethos sets a new standard today. Owning one will guarantee long lines at your telescope during any star party.

[I]f I were dropped on a desert island tomorrow with the 12-inch scope and only one eyepiece, I’d want it to be the Ethos.

Some of the views were simply stunning. The globular cluster Messier 13 in Hercules appeared as a sprawling sphere with thousands of resolved stars, many sweeping outward in sinuous arcs.

Even under the most critical examination, bright stars look sharp and round across the entire field.

The Ethos hasn’t sacrificed one bit of on-axis performance in achieving its 100° apparent field.

[T]he view of a starry sky with the Ethos and TV-NP127is is nothing short of breathtaking.

Besting the fields of other astronomical eyepieces by more than 20% in diameter and more than 50% in area, Ethos is a stunning optical achievement.


A Triple Digit Field-of-View
Read Complete S&T Review!





Ethos™: The "Majesty Factor"
The Nexus of Contrast, Power, Field
— an essay by Al Nagler

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 increases the magnification potential.

The result is an increase in what I would call the Majesty 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.
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