Title: Determinate Space Frame Telescope Structures for SNAP
1Determinate Space Frame Telescope Structures for
SNAP
- Bruce C. Bigelow
- University of Michigan
- Department of Physics
- 7/28/04
2Determinate Space Frames
- Motivations
- Minimize telescope structure deflections under
gravity - Maximize resonant frequencies on ground and
orbit - Minimize structure mass, CF outgassing, etc.
- Maximum access to optical elements (assembly,
test) - Explore parameter space for SNAP structure
3Determinate Space Frames
- Determinate space frames
- Loads carried axially (ideally)
- Deflections scale linearly with length
- d PL/AE vs. PL3/nEI
- No redundant members
- Free-body strut to node ratio S 3N 6
- Fast and easy to analyze with FEA
- May ease assembly (vs. indeterminate structures)
- Truss structures are optimal for supporting
discrete loads - Truss structures make poor fuel tanks and
fuselages
4SNAP Space Frames
- Design considerations
- Maintain symmetry to extent possible
- Locate nodes for access to primary loads
- 3 nodes above secondary mirror for hexapod mount
- 3 nodes above primary for secondary support
- 3 nodes behind primary for mirror, attach to SC
- 3 nodes below tertiary axis to stabilize
secondary supp. - Locate struts to avoid optical path
- Size struts to minimize mass and deflections
- Round struts used for constant stiffness vs.
orientation - Non-tapered struts used easy for first cut
designs - COI M55J CF used for all struts
- CF can be optimized for cross section, thermal
expansion
5SNAP Space Frames
- Design and analysis
- Still using TMA 63 optics, but results are
portable - 6 structure variants considered
- 1 selected for analysis
- Telescope mass 360kg loads, 96kg structures
- Static FEA
- Zenith pointing, gravity-release
- Dynamic FEA
- Ground test
- On-orbit, unconstrained (free-free)
6SNAP Space Frames
prtruss3 initial concept design
7Baffles fully enclose optical system, FPA
8Lower baffles removed
9Radiator removed, FPA clears 12 element (rotated)
baffle structure
10All baffles removed
11Structure is self-supporting without spacecraft
12(No Transcript)
13View from FPA side
14View from tertiary side
15Bottom view
16Top view
17Static FEA
- Static analysis
- Telescope pointed at zenith
- Parametric solid and FEA models, run in batch
mode - Optics, FPA modeled with 6 DOF solid elements
- Struts modeled with 6 DOF pipe elements
- Optics, FPA structures ignored except for mass
effects - Densities varied to match current design masses
- Primary ULE, 205 kg
- Secondary ULE, 9.7 kg, 10kg for actuators
- Fold Zerodur, 19 kg
- Tertiary ULE, 17 kg
- FPA MZT, 100 kg (no spectrograph)
18Static FEA
Elements
19Static FEA
Gz, z-axis deflections, in meters
20Static FEA
Gz, deflected shape
21Static FEA
Gz, x-axis deflections, in meters
22Static FEA
Gz, y-axis deflections, in meters
23Dynamic FEA
- Dynamic analysis
- Model and loads from static analysis
- Modal analysis for ground, launch
- f1 72 Hz
- f2 74 Hz
- f3 107 Hz
- f4 114 Hz
- f5 131 Hz
- Modal analysis for on-orbit (unconstrained)
- f7 106 Hz
- f8 107 Hz
24Static FEA
First ground mode, 72 Hz
25Static FEA
Second ground mode, 74 Hz
26Static FEA
Third ground mode, 108 Hz
27Static FEA
First free mode, 106 Hz
28Static FEA
Second free mode, 110 Hz
29Determinate Space Frames
- Conclusions
- Space frames are viable alternatives to
plate/shell structures - An space frame design for SNAP was shown and
analyzed - Many other alternatives, and combinations, exist
- The final telescope structure design will
probably result from a trade-off of multiple
requirements - Weight
- Stiffness
- Ease of modification (additional loads)
- Ease of fabrication (cost and duration)
- Ease of assembly, integration, and test
30SNAP Space Frames
prtruss1 symmetric mounts for tertiary, FPA
31SNAP Space Frames
prtruss2 hexapod tube for tertiary, FPA
32SNAP Space Frames
prtruss4 3 stacked hexapods, interferes with PM
33SNAP Space Frames
prtruss5 3 stacked hexapods, mid-level elements
intersect
34SNAP Space Frames
prtruss6 alternate support for secondary hexapod