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Hubble Space Telescope
Introduction
The Hubble Space Telescope (HST) is an example of a Cassegrain telescope. This tutorial demonstrates how to use the Conic Mirror On Axis 3D part from the Part Libraries to construct the HST Ritchey–Chrétien geometry, and how to include multiple ray release features so that rays at several field angles can be traced simultaneously. An overview of the HST is shown in Figure 1.
Figure 1: Overview of the Hubble Space Telescope.
Model Definition
Details of the Hubble Space Telescope can be found in Ref. 1 and Ref. 2. This is the nominal prelaunch design. In this tutorial the as-built details (see, for example, Ref. 3 and Ref. 4) are not considered, but additional information from these references was used to create the model. A summary of the HST parameters used in this tutorial is given in Table 1.
In this simulation the telescope geometry is constructed using two instances of the Conic Mirror On Axis 3D from the Part Libraries. The image surface is defined using a Parametric Surface primitive with the appropriate Petzval curvature. A secondary obstruction has been created using an instance of the Circular Planar Annulus 3D which can also be found in the Part Libraries. The resulting geometry sequence is shown in Figure 2.
Table 1: HUBBLE SPACE TELESCOPE PARAMeters.
Name
Value
Details
 λvac
 550 nm
Vacuum wavelength
 θx,i
Nominal x field angle, field i = 1,2,3
 θy,i
Nominal y field angle, field i = 1,2,3
 Nring
 10
Number of hexapolar rings
 Pnom
 2400.0 mm
Entrance pupil diameter
Primary mirror:
 
 Rprim
 -11040.0 mm
Primary mirror radius of curvature
 kprim
 -1.0022985
Primary mirror conic constant
 d0,prim
 2450.0 mm
Primary mirror full diameter (nominal)
 dh,prim
 600.0 mm
Primary mirror central hole diameter
 Tc,prim
 125.0 mm
Primary mirror center thickness (nominal)
Secondary mirror:
 
 Rsec
 1358.000 mm
Secondary mirror radius of curvature
 ksec
 -1.49600
Secondary mirror conic constant
 dsec
 395.0 mm
Secondary mirror diameter
 Tc,sec
 75.0 mm
Secondary mirror center thickness (nominal)
Positions:
 
 Zprim
 0 mm
Primary mirror position
 Zsec
 -4906.071 mm
Secondary mirror position
 Zbfl
 1500.0 mm
Image surface back focal length (relative to primary vertex)
 Zimage
 Zsec − Zbfl
Image surface position (relative to secondary surface)
 Misc:
 
 
 εobs
 0.33
Obstruction fraction
 Cp
Image surface Petzval curvature
Figure 2: The Hubble Space Telescope geometry sequence.
Figure 3: The Hubble Space Telescope mesh.
Results and Discussion
A ray trace has been performed at a single wavelength (550 nm) at three field angles (0, 5 and 10 arcminutes). Figure 4 shows the resulting ray trajectories; the Color Expression represents the ray positions on the image surface.
In Figure 5 the intersection of the rays with the image surface is shown. This spot diagram shows each of the three field angles, where the Color Expression is the initial radial location at the entrance pupil.
Figure 4: Ray diagram of the HST colored by radial distance from the centroid.
Figure 5: Spot diagram of the HST colored by radial distance from the center of the entrance pupil. The absolute coordinate of each spot is shown. The ring in the lower-left corner is the nominal Airy ring.
References
1. C. Burrows, Hubble Space Telescope: Optical telescope assembly handbook. Space Telescope Science Inst., Baltimore, MD, 1990.
2. D. Schroeder, Astronomical Optics. Second Edition. San Diego, CA, USA: Academic Press, 2000.
3. D. Moore and others, Final Report Hubble Independent Optical Review Panel. Goddard Space Flight Center, Greenbelt, MD, 1991.
4. L. Allen and others, The Hubble Space Telescope Optical Systems Failure Report. NASA, 1990.
Application Library path: Ray_Optics_Module/Lenses_Cameras_and_Telescopes/hubble_space_telescope
Modeling Instructions
From the File menu, choose New.
New
In the New window, click  Model Wizard.
Model Wizard
1
In the Model Wizard window, click  3D.
2
In the Select Physics tree, select Optics > Ray Optics > Geometrical Optics (gop).
3
Click Add.
4
Click  Study.
5
In the Select Study tree, select Preset Studies for Selected Physics Interfaces > Ray Tracing.
6
Click  Done.
Global Definitions
Parameters 1
1
In the Model Builder window, under Global Definitions click Parameters 1.
2
In the Settings window for Parameters, locate the Parameters section.
3
Click  Load from File.
4
Browse to the model’s Application Libraries folder and double-click the file hubble_space_telescope_parameters.txt.
Part Libraries
1
In the Geometry toolbar, click  Part Libraries.
2
In the Model Builder window, under Component 1 (comp1) click Geometry 1.
3
In the Part Libraries window, select Ray Optics Module > 3D > Mirrors > conic_mirror_on_axis_3d in the tree.
4
Click  Add to Geometry.
5
In the Select Part Variant dialog, select Specify clear aperture diameter in the Select part variant list.
6
Click OK.
Geometry 1
Primary Mirror
1
In the Model Builder window, under Component 1 (comp1) > Geometry 1 click Conic Mirror On Axis 3D 1 (pi1).
2
In the Settings window for Part Instance, type Primary Mirror in the Label text field.
3
Locate the Input Parameters section. In the table, enter the following settings:
Name
Expression
Value
Description
R
R_prim
-11.04 m
Radius of curvature (+convex/-concave)
k
k_prim
-1.0023
Conic constant
Tc
Tc_prim
0.125 m
Center thickness
d0
d0_prim
2.45 m
Mirror full diameter
d1
0
0 m
Mirror surface diameter
d_clear
0
0 m
Clear aperture diameter
d_hole
dh_prim
0.6 m
Center hole diameter
nix
nix
0
Local optical axis, x-component
niy
niy
0
Local optical axis, y-component
niz
niz
-1
Local optical axis, z-component
n_extra_a
np_extra
10
Number of extra azimuthal points
4
Locate the Position and Orientation of Output section. Find the Displacement subsection. In the zwi text field, type Z_prim.
5
Click  Build Selected.
6
Click to expand the Boundary Selections section. In the table, select the Keep checkbox for Mirror surface.
7
Click to select row number 3 in the table.
8
Click New Cumulative Selection.
9
In the New Cumulative Selection dialog, type Obstructions in the Name text field.
10
Click OK.
11
In the Settings window for Part Instance, locate the Boundary Selections section.
12
In the table, enter the following settings:
Name
Keep
Physics
Contribute to
Mirror rear surface
 
√
Obstructions
Mirror edges
 
√
Obstructions
Secondary Mirror
1
In the Geometry toolbar, click  Part Instance and choose Conic Mirror On Axis 3D.
2
In the Settings window for Part Instance, type Secondary Mirror in the Label text field.
3
Locate the Input Parameters section. In the table, enter the following settings:
Name
Expression
Value
Description
R
R_sec
1.358 m
Radius of curvature (+convex/-concave)
k
k_sec
-1.496
Conic constant
Tc
Tc_sec
0.075 m
Center thickness
d0
d_sec
0.395 m
Mirror full diameter
d1
0
0 m
Mirror surface diameter
d_clear
0
0 m
Clear aperture diameter
d_hole
0
0 m
Center hole diameter
4
Locate the Position and Orientation of Output section. Find the Coordinate system to match subsection. From the Take work plane from list, choose Primary Mirror (pi1).
5
From the Work plane list, choose Mirror vertex intersection (wp1).
6
Find the Displacement subsection. In the zwi text field, type Z_sec.
7
Click  Build Selected.
8
Locate the Boundary Selections section. In the table, enter the following settings:
Name
Keep
Physics
Contribute to
Mirror surface
√
√
None
Mirror rear surface
 
√
Obstructions
Mirror edges
 
√
Obstructions
Image Surface
A parametric surface can be used to define the image surface.
1
In the Geometry toolbar, click  More Primitives and choose Parametric Surface.
2
In the Settings window for Parametric Surface, type Image Surface in the Label text field.
3
Locate the Parameters section. Find the First parameter subsection. In the Minimum text field, type -hw_image.
4
In the Maximum text field, type hw_image.
5
Find the Second parameter subsection. In the Minimum text field, type -hw_image.
6
In the Maximum text field, type hw_image.
7
Locate the Expressions section. In the x text field, type s1.
8
In the y text field, type s2.
9
In the z text field, type Cp*(s1^2 + s2^2)/(1 + sqrt(1 - Cp^2*(s1^2 + s2^2)))*1[m]. This is the equation of a sphere having a curvature Cp. This is the Petzval curvature defined in the Parameters node.
10
Locate the Position section. In the z text field, type Z_image.
11
Locate the Coordinate System section. From the Take work plane from list, choose Secondary Mirror (pi2).
12
From the Work plane list, choose Mirror vertex intersection (wp1).
13
Locate the Selections of Resulting Entities section. Select the Resulting objects selection checkbox.
Part Libraries
The secondary mirror mount creates an obstruction.
1
In the Geometry toolbar, click  Part Libraries.
2
In the Model Builder window, click Geometry 1.
3
In the Part Libraries window, select Ray Optics Module > 3D > Apertures and Obstructions > circular_planar_annulus in the tree.
4
Click  Add to Geometry.
Geometry 1
Secondary Obstruction
1
In the Model Builder window, under Component 1 (comp1) > Geometry 1 click Circular Planar Annulus 1 (pi3).
2
In the Settings window for Part Instance, type Secondary Obstruction in the Label text field.
3
Locate the Input Parameters section. In the table, enter the following settings:
Name
Expression
Value
Description
d0
d0_obs
0.792 m
Diameter, outer
d1
0
0 m
Diameter, inner
4
Locate the Position and Orientation of Output section. Find the Coordinate system to match subsection. From the Take work plane from list, choose Secondary Mirror (pi2).
5
From the Work plane list, choose Mirror vertex intersection (wp1).
6
Find the Displacement subsection. In the zwi text field, type Z_obs.
7
Locate the Boundary Selections section. In the table, enter the following settings:
Name
Keep
Physics
Contribute to
All
 
√
Obstructions
8
Click  Build Selected.
9
Click the  Go to Default View button in the Graphics toolbar.
10
Click the  Orthographic Projection button in the Graphics toolbar.
11
Click the  Zoom Extents button in the Graphics toolbar. Compare the resulting geometry to Figure 2.
Geometrical Optics (gop)
1
In the Model Builder window, under Component 1 (comp1) click Geometrical Optics (gop).
2
In the Settings window for Geometrical Optics, locate the Domain Selection section.
3
Click  Clear Selection.
4
Locate the Ray Release and Propagation section. In the Maximum number of secondary rays text field, type 0.
Primary
1
In the Physics toolbar, click  Boundaries and choose Mirror.
2
In the Settings window for Mirror, type Primary in the Label text field.
3
Locate the Boundary Selection section. From the Selection list, choose Mirror surface (Primary Mirror).
Secondary
1
In the Physics toolbar, click  Boundaries and choose Mirror.
2
In the Settings window for Mirror, type Secondary in the Label text field.
3
Locate the Boundary Selection section. From the Selection list, choose Mirror surface (Secondary Mirror).
Obstructions
1
In the Physics toolbar, click  Boundaries and choose Wall.
2
In the Settings window for Wall, type Obstructions in the Label text field.
3
Locate the Boundary Selection section. From the Selection list, choose Obstructions.
4
Locate the Wall Condition section. From the Wall condition list, choose Disappear.
Image
1
In the Physics toolbar, click  Boundaries and choose Wall.
2
In the Settings window for Wall, type Image in the Label text field.
3
Locate the Boundary Selection section. From the Selection list, choose Image Surface.
Release from Grid 1
Next, create three release features for each of the field angles defined in the Parameters node.
1
In the Physics toolbar, click  Global and choose Release from Grid.
2
In the Settings window for Release from Grid, locate the Initial Coordinates section.
3
From the Grid type list, choose Hexapolar.
4
Specify the qc vector as
-dx1
x
-dy1
y
dz
z
5
Specify the rc vector as
0
x
0
y
1
z
6
In the Rc text field, type P_nom/2.
7
In the Nc text field, type N_ring.
8
Locate the Ray Direction Vector section. Specify the L0 vector as
vx1
x
vy1
y
-vz
z
Release from Grid 2
1
Right-click Release from Grid 1 and choose Duplicate.
2
In the Settings window for Release from Grid, locate the Initial Coordinates section.
3
Specify the qc vector as
-dx2
x
-dy2
y
4
Locate the Ray Direction Vector section. Specify the L0 vector as
vx2
x
vy2
y
Release from Grid 3
1
Right-click Release from Grid 2 and choose Duplicate.
2
In the Settings window for Release from Grid, locate the Initial Coordinates section.
3
Specify the qc vector as
-dx3
x
-dy3
y
4
Locate the Ray Direction Vector section. Specify the L0 vector as
vx3
x
vy3
y
Mesh 1
In the Model Builder window, under Component 1 (comp1) right-click Mesh 1 and choose Build All. The mesh should looks like Figure 3.
Study 1
Step 1: Ray Tracing
1
In the Model Builder window, under Study 1 click Step 1: Ray Tracing.
2
In the Settings window for Ray Tracing, locate the Study Settings section.
3
From the Time-step specification list, choose Specify maximum path length.
4
In the Lengths text field, type 0 17. This path length is sufficient to ensure that all rays reach the image plane.
5
In the Study toolbar, click  Compute.
Now, create a ray diagram.
Results
Ray Diagram
1
In the Settings window for 3D Plot Group, type Ray Diagram in the Label text field.
2
Click to expand the Title section. From the Title type list, choose None.
3
Locate the Color Legend section. Select the Show maximum and minimum values checkbox.
4
Select the Show units checkbox.
5
In the Model Builder window, expand the Ray Diagram node.
Color Expression 1
1
In the Model Builder window, expand the Results > Ray Diagram > Ray Trajectories 1 node, then click Color Expression 1.
2
In the Settings window for Color Expression, locate the Expression section.
3
In the Expression text field, type at('last',gop.rrel). This is the radial coordinate relative to the centroid at the image plane for each release feature.
4
From the Unit list, choose µm.
Surface 1
1
In the Model Builder window, right-click Ray Diagram and choose Surface.
2
In the Settings window for Surface, locate the Coloring and Style section.
3
From the Coloring list, choose Uniform.
4
From the Color list, choose Gray.
Selection 1
1
Right-click Surface 1 and choose Selection.
2
In the Settings window for Selection, locate the Selection section.
3
From the Selection list, choose Obstructions.
Surface 2
1
In the Model Builder window, right-click Ray Diagram and choose Surface.
2
In the Settings window for Surface, locate the Coloring and Style section.
3
From the Coloring list, choose Uniform.
4
From the Color list, choose Custom.
5
On Windows, click the colored bar underneath, or — if you are running the cross-platform desktop — the Color button.
6
Click Define custom colors.
7
Set the RGB values to 189, 201, and 216, respectively.
8
Click Add to custom colors.
9
Click Show color palette only or OK on the cross-platform desktop.
Selection 1
1
Right-click Surface 2 and choose Selection.
2
Select Boundaries 4 and 11 only.
3
In the Ray Diagram toolbar, click  Plot.
4
Click the  Zoom Extents button in the Graphics toolbar. Compare the resulting image to Figure 4.
Spot Diagram
Next, create a spot diagram.
1
In the Results toolbar, click  2D Plot Group.
2
In the Settings window for 2D Plot Group, type Spot Diagram in the Label text field.
3
Locate the Color Legend section. Select the Show units checkbox.
Spot Diagram 1
1
In the Spot Diagram toolbar, click  More Plots and choose Spot Diagram.
2
In the Settings window for Spot Diagram, locate the Layout section.
3
From the Layout list, choose Rectangular grid.
4
In the Horizontal padding factor text field, type 0.
5
Click to expand the Annotations section. Select the Show circle checkbox.
6
In the Radius text field, type r_Airy.
Color Expression 1
1
Right-click Spot Diagram 1 and choose Color Expression.
2
In the Settings window for Color Expression, locate the Expression section.
3
In the Expression text field, type at(0,gop.rrel). This is the radial coordinate relative to the centroid at the entrance pupil for each ray release.
4
In the Spot Diagram toolbar, click  Plot.
5
Click the  Zoom Extents button in the Graphics toolbar. Compare the resulting image to Figure 5.