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Roberto Ragazzoni INAF – Astronomical Observatory of Padova [email protected] Feasibility of the aspheric lens Catania, June 11 2014 On behalf and with extensive inputs from the Telescope Group (D. Magrin, D. Piazza, W. Benz, J. Farinato, S. Basso, M. Ghigo, M. Munari, P. Spano’, G. Piotto, M. Barbieri, E. Pace, S. Scuderi, I. Pagano, L. Gambicorti, C. Arcidiacono, R.U. Claudi, V. Viotto, M. Dima, G. Gentile, R. Canestrari, S. Desidera, S. Benatti)
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Roberto Ragazzoni INAF – Astronomical Observatory of Padova [email protected]

Feb 24, 2016

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Page 1: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Roberto RagazzoniINAF – Astronomical Observatory of [email protected]

Feasibility of the aspheric lensCatania, June 11 2014

On behalf and with extensive inputs from the Telescope Group (D. Magrin, D. Piazza, W. Benz, J. Farinato, S. Basso, M. Ghigo, M. Munari, P. Spano’, G. Piotto, M. Barbieri, E. Pace, S. Scuderi, I. Pagano, L. Gambicorti, C. Arcidiacono, R.U.

Claudi, V. Viotto, M. Dima, G. Gentile, R. Canestrari, S. Desidera, S. Benatti)

Page 2: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Roberto RagazzoniINAF – Astronomical Observatory of [email protected]

Feasibility of the aspheric lensCatania, June 11 2014

On behalf and with extensive inputs from the Telescope Group (D. Magrin, D. Piazza, W. Benz, J. Farinato, S. Basso, M. Ghigo, M. Munari, P. Spano’, G. Piotto, M. Barbieri, E. Pace, S. Scuderi, I. Pagano, L. Gambicorti, C. Arcidiacono, R.U.

Claudi, V. Viotto, M. Dima, G. Gentile, R. Canestrari, S. Desidera, S. Benatti)

This is still the “old” PLATO 1.0 group

Page 3: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

The aspheric issue…

We have been asphericized by an hard life (thank you Silvio…)

We had two offers from manufacturer for actually making one (in S-FPL51) for test (SESO & Silo)

We have a detailed plan and feasibility by Sagem-Reosc that already manufactured two similar sets for a different space project (and they made similar comments as Zeiss quotation in RUAG report!)

ESA challenged themselves to improve Thales design to achieve performances and found they need two aspherics

Asphere is on a lens with one flat surface MediaLario is testing their manufacturing

abilities on glass S-FPL51

From a summarizing slide of June 15, 2011 (3 yers ago…)

Page 4: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

The aspheric issue…

We have been asphericized by an hard life (thank you Silvio…)

We had two offers from manufacturer for actually making one (in S-FPL51) for test (SESO & Silo)

We have a detailed plan and feasibility by Sagem-Reosc that already manufactured two similar sets for a different space project (and they made similar comments as Zeiss quotation in RUAG report!)

ESA challenged themselves to improve Thales design to achieve performances and found they need two aspherics

Asphere is on a lens with one flat surface MediaLario is testing their manufacturing

abilities on glass S-FPL51

From a summarizing slide of June 15, 2011 (3 yers ago…)

Page 5: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

The team background

Rosetta Wide Angle Camera design An off-axis tilted FoV design with

aspheric mirrors Emphasys was on detection of faint

gasesous features from comet nuclei Clean PSF: unobstructed pupil,

monochromatic and low scatter designNone of the above does apply to

PLATO!Several ground based 4m and 8m

class instruments (all with aspheric surfaces)

Page 6: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Postcards sent around…

Page 7: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Postcards sent around…

Two of the lens has an aspheric surface

surprisingly similar in size and deviation!

Page 8: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Impact of increasing aperture & FOV on Thales optical design for Plato.

January 2010Isabel Escudero

Page 9: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Purpose of study.

Modify Thales design as follows: Entrance aperture diameter: 15% bigger. FOV: from a circle of 28º diameter to a

square of 28º side length. Image: quality equivalent to that of

Thales design for the whole new FOV (criterion is 90% EEC diameter)

Focal length: same as original Add Fused Silica plate in front Aspherics necessary?

Page 10: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Comparing sizes.10:01:23

plato_thales ME 11-Jan-10

50.00 MM

10:11:01

Science 15-Jan-10

50.00 MM

15:48:36

plato_v10 ME 08-Jan-10

50.00 MM

15:49:37

plato_v20 ME 08-Jan-10

50.00 MM

Thales Science

Plato_v10 Plato_v20

Page 11: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Comparing performance

Design Field object (degrees) Diameter of 90% encircled energy (µm) Plato_Thales Axis/9.6/13.7º/19.6º 34.8 / 42.6 / 58.9 / NA Plato_v10 Axis/9.6/13.7º/19.6º 39.7 / 34.4 / 41.8 / 65.8 Plato_v20 Axis/9.6/13.7º/19.6º 31.9 / 34.0 / 42.8 / 59.6

System EPD (mm) EFL(mm) FOV Thales 83 239.5 28º diameter circle Science 120 247.5 28º diameter circle Plato_v10/Plato_v20 95.45 239.5 28º side square

Design Field Object Incidence Angle at image Distortion (%) Plato_Thales 14º 26.7º 0.7 Plato_v10 19.6º 38.3º 0.7 Plato_v20 19.6º 38º 2.0 Science 14º 31º 2.9

Page 12: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Conclusions: Thales_v10/_v20. Two aspheric surfaces are required for

larger EP & FOV. If FOV = 28º diameter circle, one aspheric

surface is enough. Fused silica plate becomes a lens:

curvatures and aspheric are needed. Note values of distortion (=> calibration

and post-processing for field superposition).

Note large angles of edge field object at image plane: relevant for radiometry.

Page 13: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Conclusion by ESA…

Page 14: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Do we need aspheres…?

Yes… Accordingly to ESA (upgrading of THALES design)

at least two; With our own design (actually all the “last”

versions) just one.

Page 15: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Feasibility strategy

ESA never questioned feasibility of one TOU

ESA often being concern about “mass” (well, sort of…) production

Construction is one of the issues..We focus on demonstrating a fast

procedure (less than one week) in the warm…

Aggressive plan to demonstrate we can handle CaF optical elements

Page 16: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Frame connected to the bench, allowing the rotation for lenses insertion from the top and their alignment similarly to what would happen with the final structure, withthe possibility to be rotated of 180º to insertthe lenses from both sides(L3 will be the first one)

TOU BreadBoard

Rotating points

TOU Dummy Structure

Laser

Beam Expander

Iris1

B/S

Back Reflected Light

Transmitted Light

CCD

CCD

Iris2

Page 17: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it
Page 18: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Alternative designs

A design with an aspheric CaF (because SESO claimed that with some manufacturing process that would be easier/cheaper/faster)

A design CaF-free (in case we fail space qualification of CaF lens)

A design taking into account the common directives of manufacturer

Page 19: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Design 4

BK7 G18CaF2

CaF2N-KZFS11 S-FPL53 KZFSN5

BK7

Page 20: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Design 4 - EE

90%EE<30×30 arcsec2 ~ 2×2 pixels2

90%EE<37.5×37.5 arcsec2 ~ 2.5×2.5 pixels2

90%EE<45×45 arcsec2 ~ 3×3 pixels2

2×2 pixels2

Page 21: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Design 5

BK7 G18S-FPL51

N-KZFS11S-FPL53 KZFSN5

BK7

S-FPL51

Page 22: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Design 5 - EE

2×2 pixels2

90%EE<30×30 arcsec2 ~ 2×2 pixels2

90%EE<37.5×37.5 arcsec2 ~ 2.5×2.5 pixels2

90%EE<45×45 arcsec2 ~ 3×3 pixels2

Page 23: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Baseline - EE

90%EE<30×30 arcsec2 ~ 2×2 pixels2

90%EE<37.5×37.5 arcsec2 ~ 2.5×2.5 pixels2

90%EE<45×45 arcsec2 ~ 3×3 pixels2

Page 24: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

The CaF issue…

Already flown… One company (SESO) would prefer as

asphere Baseline design has CaF in the spherical,

smallest and more protected position (L3) We have in our hand a produced L3

identical to the flight one (assuming baseline)

We have two blanks similar in size, glued to the same holder and cured in two different ways now in CNES and UniBern for thermal and vibration tests…

We have an acceptable, although not brilliant, B plan CaF-less

Page 25: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Foreseen Activities (CaF2):Shipped blank to

PDShipped to SGGluing blankCuring (th.cycle)Shipped to PDShipped to UniBEVibratingShipped to CNESThermal cycling

Shipped blank to PD

Shipped to SGGluing blankShipped to PDShipped to CNESThermal cycling

Survived!

Survived!

Remember that L3 in the BB

is made in CaF2 as well!

Page 26: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it
Page 27: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Foreseen Activities (BB):

Mounting lenses on mounts (gluing) Aligning within tolerances Testing the “warm” optical quality

interferometrically Measuring the “warm” PSF directly Measuring the “warm” PSF via Hartmann Measuring the “cold” PSF directly Measuring the “cold” PSF via Hartmann Validation or lessons learned of the

alignment process

DONE !!!

Page 28: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

One aspheric done on purpose…

Page 29: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Various studies issued…

Page 30: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Various studies issued…

Page 31: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Production plans…

Page 32: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Production plans…

Page 33: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Production plans…

Page 34: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it
Page 35: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

Summary…Selex: Ok with industrial planSagem/Reosc: Ok with industrial planMediaLario: Interested, feasibility Ok, now joining

Selex?Seso: Ok but would prefer CaF2 (technology driven)RUAG: Market analysis…

Zeiss: doable, delivery time non critical Asphericon: doable at the limit (delivery time) of their

abilities Steinbeis TransferZentrum: identified several

technologies Leica: doable, but reccomending harder material Fisba: they do not have capabilities (in spite of…) PrazisionOptik: they do not make aspheres SwissOptics: they think are doable but exceed the size they

handle

Page 36: Roberto Ragazzoni INAF – Astronomical Observatory of  Padova roberto.ragazzoni@inaf.it

What is next…?

Regain informal contact with all industries (some already made on their own… Sagem & MediaLario)

Select one or two for an updated formal adjourned contact

Place the accent on the serial and industrial production

Take –very fastly- a final choice as the overall baseline based on existing informations