Title: Apophis Mitigation
1Apophis Mitigation Research Project
Project Kickoff Meeting February 9, 2009
2- Research Project Announcement
- This project will continue the efforts of the
Aero 426, Space System Design (Fall, 2008), class
to develop a space mission that will rendezvous
with the dangerous Near Earth Asteroid (NEA)
99942 Apophis and apply various technologies to
deflect its orbit from possible Earth impact
before its next close encounter on Friday, 13
April, 2029. Because of the long lead time
required for orbit deflection, a mature design
concept for the Deflect Apophis System (DAS) must
be developed within the next two years. This is
an ongoing collaboration with NASA Ames and is
being conducted with international support. - Starting with the notional design developed in
Aero 426, research participants will - (1) Travel to NASA Ames, near San Francisco, to
work in their concurrent engineering design
facility for 3 to 5 days, developing a firm
baseline design, - (2) Respond to the National Research Councils
(NRCs) Announcement of opportunity dated
December 17 and submit a full proposal to the NRC
by March 20, 2009. For further details, see - http//www7.nationalacademies.org/ssb/NEO_surveys
_mitigation.htmlP16_19 - (3) Conduct prototype development of an asteroid
deflection technology and test it experimentally. - The above steps will be conducted during the
spring, 2009 semester and will lead to
preparation of a proposal (jointly with NASA
Ames) to NASA HQ for a Discovery-class mission
during the summer of 09. These activities will
contribute significantly to our understanding of
how to mitigate the potential hazards of NEAs. - We solicit the participation of junior and senior
undergraduate students and graduate students.
Students from all departments of engineering and
science are encouraged to participate. Finally,
qualified and effective participants will be
offered summer employment. - For further information and to volunteer your
participation, contact - Dr. David C. Hyland
- Professor of Aerospace Engineering, Wisenbaker
Chair of Engineering, - Dwight Look College of Engineering
3Apophis Mitigation Project Kickoff - Agenda
- Introduction to Apophis
- Project History
- Outline of Design concepts to-date
- Three activities
- Proposal to NRC
- Albedo change technology
- Baseline design definition (at NASA Ames)
- Schedule of activities
4Apophis 99942 Background Information
Project Background
- Discovered on June 19th, 2004 by R. A. Tucker, D.
J. Tholen and F. Bernardi at Kitt Peak - Orbital models have identified several close
Earth approaches, occurring roughly every 7
years. When Apophis passes by in 2029 it could
pass through a gravitational keyhole which would
swing Apophis into a collision path with Earth in
2036 - As an Aten class NEA, Apophis rated as high as 4
on the Torino scale but has been downgraded to a
0 as its probability of impact in 2029 has been
commonly accepted at 1/45,000
Source http//neo.jpl.nasa.gov/apophis
AAA System Design Review
4
December 9, 2008
5Apophis 99942 Physical Data
Project Background
- LL-chondrite composition
- Estimated rotational period of 30.57 h
- Keyhole Event April 13, 2029
- Results in resonant return and possible impact in
April 2036
Sources http//ssd.jpl.nasa.gov/sbdb.cgi?sstr999
42orb1cov0log0discovery
Chesley, Milani, Vokrouhlicky, Icarus 148,
118138 (2000)
5
AAA System Design Review
December 9, 2008
6APEP
Project Background
- Agencies from around the world, including
NASA/JPL, Caltech, and Arecibo, have analyzed and
identified Apophis orbital elements and physical
properties with limited levels of accuracy - Uncertainty in the effects from albedo and
gravitational forces over time are again causing
concern about a potential impact with Earth - The Fall 07 426, Spring 08 401 and Fall 08 402
classes started the design of the Apophis
Preliminary Exploration Platform (APEP) mission.
Objectives were - Rendezvous with Apophis in 2013, act as a beacon
to enable precise tracking, - Measure physical characteristics most relevant to
improved accuracy of orbit prediction. - If Apophis is on a collision course with Earth
and planning of a mitigation mission is started
after APEP discovers this fact, changing the
course of the asteroid may be impossible.
AAA System Design Review
6
December 9, 2008
77
AAA - System Concept Briefing
December 3, 2008
8AAA - System Concept Briefing
8
December 3, 2008
9Apophis Preliminary Exploration Platform (APEP)
Mission Statement
- The APEP mission is to rendezvous with the near
earth asteroid Apophis 99942 to conduct a study
of physical characteristics and accurately track
the orbit in order to determine the probability
of an Earth impact in 2036.
9
AAA - System Concept Briefing
December 3, 2008
10Top-Level Mission Profile
Maintain 3 km standoff distance from Apophis for
1 year
Launch APEP mission by 2012
Rendezvous with Apophis after 1 year travel time
Broken-Plane Maneuver to minimize overall ?V
Relay data to ground stations on Earth to
determine Apophis tracking and science
10
AAA - System Concept Briefing
December 3, 2008
11Events in the APEP Project History
- Aero 426 (Fall, 2007) students formulated
notional mission design with final presentation
in December 2007. - Project continued in spring semester as the focus
of the two-semester capstone design sequence Aero
401-402, Spacecraft Design. - January 28 30, 2008 Aggies Against Apophis
(AAA) team travels to the Jet Propulsion Lab to
conduct concurrent engineering design sessions
with Team X. - Result Baseline design serving as the starting
point for Aero 401 - February 2008 Educational partnership with King
Abdullaziz City for Science and Technology
(KACST) initiated. - KACST personnel join the AAA team, undertake to
provide design development of APEP Science
Instruments - Spring 2008 semester AAA team (Aero 401)
refines baseline to develop conceptual design. - Fall 2008 semester AAA team (Aero 402) travels
to AMES research center to present current
design. - The result is a partnership with AMES for a
proposal effort to NASA HQ - Formal AM / NASA Ames / KACST partnership under
negotiation.
11
AAA - System Concept Briefing
December 3, 2008
12(No Transcript)
13(No Transcript)
14Rationale for Exploration and Mitigation Mission
Launch Dates
Project Background
2015
2010
2020
2025
2040
2035
2030
We are too late for the 2012 launch. We must
amalgamate the exploration and mitigation
missions for the later launch window.
AAA System Design Review
14
December 9, 2008
15Apophis Deflection System
Project Background
- The challenge facing the fall 08, 426 class was
to develop a system that can sufficiently modify
the trajectory of Apophis such that it will not
impact the Earth in 2036. - A subsidiary goal is to design the spacecraft
such that it can be fabricated and tested in the
AggieSat Laboratory. - The class was originally split into four teams.
Each team examined multiple methods of
deflection, including but not limited to - Gravity Tractor
- Solar Sublimation
- Kinetic Impactor
- Electric Propulsion Devices
- Albedo Modification Systems
- Nuclear Burst
- Each team then investigated one method in depth
and presented the method to the rest of the
class. The best design was chosen as the system
that would be developed by the whole class as a
unified team. - The Gravity Tractor was chosen as the best design
and therefore is the focus of this presentation. - Albedo modification is being investigated as a
secondary mitigation technique.
AAA System Design Review
15
December 9, 2008
16Deflect Apophis System(DAS) Mission Statement
- The DAS mission is to intercept the near-Earth
asteroid Apophis 99942 and perturb its orbit to
prevent an Earth impact in 2036.
AAA Conceptual Design Review
16
April 21, 2008
April 21, 2008
17Mission Overview
Top-Level Mission Profile
Maintain 400 m standoff distance from Apophis
for 4 years Deflect via Gravity Tractor effect
Deploy albedo altering experiment during
mitigation
Launch DAS mission by 2022
Rendezvous with Apophis after 5 month travel
time
Relay data to ground stations on Earth to
determine mitigation effectiveness
17
AAA System Design Review
December 9, 2008
18Gravity Tractor Concept
Mitigation, Payload, Telecom, and Instruments
- Use Newtons Law of Universal Gravitation
- Use a spacecraft to impart a gravitational force
upon Apophis to gently move Apophis to a
non-Earth impacting orbit - Utilize the 2029 flyby to enhance mitigation
efforts - Small changes pre-flyby result in large changes
in Apophis trajectory post-flyby
18
AAA System Design Review
December 9, 2008
19Albedo Change
Mitigation, Payload, Telecom, and Instruments
- Any change in albedo alters solar pressure and
the Yarkovsky effect - Fmax 0.70 N from solar pressure and Yarkovsky
effect - Orbit Deviation (assuming 25 kg coating)
- By 2036, a 4 change in albedo (beginning in
2018) will deflect Apophis between 17 and 45
Earth radii - Model based on comparison with results of Chesley
paper
AAA System Design Review
19
December 9, 2008
20- Documentation on the design work to-date has been
placed on the web. Go to - aeweb.tamu.edu\aero489
- Open folder Apophis Mitigation Project
21Planned Activities
- Three main activities
- Respond to the NRC AO with a mitigation proposal
(due March 20) - Conduct technology maturation experiments
- Albedo change deflection technology Design and
fab the albedo change dispense mechanism Test in
the STC vacuum chamber - Working at NASA Ames project design center,
complete definition of baseline design.(Teamed
with NASA Ames, submit proposal to NASA HQ for a
Discovery-Class mission (Summer, 2009))
22Activity 1 Submit proposal to the NRC
23Letter of Intent Submitted to the NRC
Authoring Organization Name Texas AM
University, Dwight Look College of Engineering,
College of Science Description of Proposed
Solution This is a mission concept for
mitigating NEOs. We deflect the orbit of a NEO
away from Earth collision by a near-term
application of the gravity tractor approach,
followed by an albedo modification technique. The
former method is well-known and can be applied
immediately upon the spacecrafts arrival at the
NEO since detailed knowledge of the physical
properties of the NEO is not required. During
gravity tractoring, on-board instruments
determine the spin state, and thermal
characteristics of the NEO in sufficient detail
to model the Yarkovsky effect. With this data, we
apply a novel albedo change device that
dispenses, in a controlled fashion, ionized
powder to selected regions of the NEO surface
which is itself ionized by ultraviolet radiation.
Electrostatic attraction provides the dominant
force that will distribute and bind the powder to
the surface. The author and his AM students have
defined a reference mission to the asteroid 99942
Apophis. We show that a 4 albedo change
(beginning in 2018), using 25 kg of surfacing
material, will deflect Apophis between 17 and 45
Earth radii by 2036, depending on the spin state.
Note that whereas gravity tractoring is of
limited duration, the albedo change treatment can
operate forever.
24Activity 2 Design, Fab Lab Test of Albedo
Change Mechanism
- After review of previous work, we brainstorm a
variety of albedo change techniques - Choose one idea
- Is it mechanically simple?
- Is it dynamically simple?
- Is it operationally simple?
- Is it low mass, low cost and effective?
- For the chosen concept
- Analyze performance
- Identify areas of technical uncertainty
- Define experiment (s) to retire uncertainty
- Fab and test
- Document test results for our proposal to NASA HQ
25Albedo Treatment Options
Mitigation, Payload, Telecom, and Instruments
- Paint
- Heavy
- Difficult to apply
- Freezing possible
- Chalk
- Lightweight
- May coat unevenly
- Reflective Sheet
- Very large
- Difficult to open and deploy onto surface
- Glass Beads
- Heavy
- May be covered by dusty surface
- Easy to carry and release
AAA System Design Review
25
December 9, 2008
26Albedo Change Mechanism
26
AAA System Design Review
December 9, 2008
27Activity 3 Completion of Baseline Mission Concept
- Review previous work on the exploration and
mitigation missions - Students will be organized into the following
technical specialty teams - Albedo Change Subsystem
- Exploration Science Instruments Proximity
Operations - Telecom, Tracking CDH sub-systems
- Trajectory, Propulsion, Attitude Control System
- Structures, Thermal, and Power
- Budget and Scheduling
- Each team is to identify design holes in its
area. These define the issues that are to be
addressed in the concurrent engineering design
session at NASA Ames - Perform conceptual design at NASA Ames during
the week of April 6, 2009
28Schedule of Activities
- Feb. 9 Kickoff meeting (All)
- Pass out Technical Specialty Group
questionnaires (DCH), - Solicit candidates for Program Manager
Assistant Program Manager (DCH) - Feb. 16 Review of design work to-date (DCH)
- Feb. 20 Return completed Technical Specialty
Group questionnaires (AAA) - Finish reviewing 426 and 402 Final Presentations
(AAA) - Feb. 23 Review thermal emission effects (DCH)
- Assign technical specialty groups (DCH)
- Elect PM and APM (AAA)
- Feb. 23-27 Brainstorm albedo change mechanism
ideas (All) - Formulate amalgamated mission concept (AAA
technical teams) - March 2 Select, albedo change device concept
(All) - NRC proposal outline assignment of
responsibilities (DCH) - March 9 Proposal progress review (All)
- Albedo change technology experiment definition
(AAA albedo change team) - March 16 Proposal Progress review (All)
- March 20 Submit proposal to NRC
29Schedule of Activities - Continued
- March 23 Define holes in mission design (AAA
technical teams) - March 23 - April 3 Work on albedo change
technology experiment (AAA albedo team DCH) - Finish defining design holes to be filled at
NASA Ames design session (AAA technical teams) - March 30 Progress review/ prep for NASA Ames
(All) - Complete technology experiment (AAA albedo team)
- April 6 Final prep for Ames visit
- April 8-10 Work at NASA Ames concurrent
engineering design facility - April 13 Baseline design results review (All)
- April 20 Final Presentation
-
30FINI
FINI
Alternate system offered was the Atlas 2 with
4.2m fairing at a cost of 84M Presenters were
uncertain about this. MIT presentation material
quotes a diameter of 1.49m