australian centre for space photonics andrew mcgrath anglo-australian observatory

Australian Centre for Space PhotonicsAustralian Centre for Space Photonics

Andrew McGrath

Anglo-Australian Observatory

This PresentationThis Presentation

Interplanetary communications problem

Long term solutionHistorical Australian involvementFurther Australian involvementMaking it happen

Exploration of MarsExploration of Mars

Highlights the communications problem

Long term and substantial past and continuing international investment

Exploration of MarsExploration of Mars 1960 Two Soviet flyby attempts 1962 Two more Soviet flyby attempts,

Mars 1 1964 Mariner 3, Zond 2 1965 Mariner 4 (first flyby images) 1969 Mariners 6 and 7 1971 Mariners 8 and 9 1971 Kosmos 419, Mars 2 & 3 1973 Mars 4, 5, 6 & 7 (first landers) 1975 Viking 1, 1976 Viking 2

Exploration of MarsExploration of Mars

1988 Phobos 1 and 2 1992 Mars Observer 1996 Mars 96 1997 Mars Pathfinder, Mars Global Surveyor 1998 Nozomi 1999 Climate Orbiter, Polar Lander and Deep

Space 2 2001 Mars Odyssey

Planned Mars ExplorationPlanned Mars Exploration

2003 Mars Express 2004 Mars Exploration Rovers 2005 Mars Reconnaissance Orbiter 2007+ Scout Missions 2007 2009 Smart Lander, Long Range Rover 2014 Sample Return

Interplanetary CommunicationInterplanetary Communication

Radio (microwave) links, spacecraft to Earth

Newer philosophy - communications relay (Mars Odyssey, MGS)

Sensible network topology25-W X-band (Ka-band experimental)

<100 kbps downlink

Communications BottleneckCommunications Bottleneck

Current missions capable of collecting much more data than downlink capabilities (2000%!)

Currently planned missions make the problem 10x worse

Future missions likely to collect ever-greater volumes of data


Increasing downlink rates critical to continued investment in planetary exploration


NASA's perception of the problem is such that they are considering an array of 3600 twelve-metre dishes to accommodate currently foreseen communications needs for Mars alone

Communications Energy BudgetCommunications Energy Budget

Consider cost of communications reduced to transmitted energy per bit of information received


• information proportional to number of photons (say, 10 photons per bit)• diffraction-limited transmission so energy density at receiver proportional to (R/DT)-2

• received power proportional to DR2

• photon energy hc /

So:

Cost proportional to R2 / (DT2DR

2)

Assumptions:


Cost proportional to R2 / (DT2DR

2)

X-band transmitter ~ 40 mmLaser transmitter ~ 0.5-1.5 m

Assuming similar aperture sizes and efficiencies, optical wins over microwave by > 3 orders of magnitude

Long-term SolutionLong-term Solution

Optical communications networksAdvantages over radioHigher modulation ratesMore directed energyAnalagous to fibre optics vs. copper

cables

Lasers in SpaceLasers in Space

Laser transmitter in Martian orbit with large aperture telescope

Receiving telescope on or near EarthPreliminary investigations suggest

~100Mbps achievable on 10 to 20 year timescale

Enabling technologies require accelerated development

Key TechnologiesKey Technologies

Suitable lasersTelescope tracking and guidingOptical detectorsCost-effective large-aperture

telescopesAtmospheric propertiesSpace-borne telescopes

An Australian Role - till nowAn Australian Role - till now

History of involvementLaunch sitesDevelopment of early satellitesCommunications– Deep Space Network– Parkes, ATNF– Continuing involvement

An Australian Role - in the futureAn Australian Role - in the future

Australian organisations have unique capabilities in the key technologies required for deep space optical communications links

High-power, high beam quality lasers Holographic correction of large telescopes Telescope-based instrumentation Telescope tracking and guiding

The University of AdelaideThe University of Adelaide

Optics Group, Department of Physics and Mathematical Physics– High power, high beam quality, scalable

laser transmitter technology – Holographic mirror correction – Presently developing high power lasers

and techniques for high optical power interferometry for the US Advanced LIGO detectors

Anglo-Australian ObservatoryAnglo-Australian Observatory

Telescope technology Pointing and tracking systems Atmospheric transmission (seeing,

refraction) Cryogenic and low noise detectors Narrowband filter technology

Macquarie UniversityMacquarie University

Centre for Lasers and Applications– Optical communications – Transmitter technology

A ProposalA Proposal

Use the ARC 'Centre of Excellence' programme to link these organisations to capitalise on Australia's strategic advantages to become an indispensable partner in the world-wide scientific space exploration effort


To expand unique Australian capabilities and experience to progress research into key technologies for an interplanetary high-data rate optical communications link that are synergistic with near term space communication needs.


Manage a portfolio of research projects in the key technologies for an interplanetary optical communications link

Work in close collaboration with overseas organizations such as NASA and JPL

An Australian foothold into the well-established `big science' investment of the leading space agencies


Closer ties to leading space agencies and their current and planned missions


Australia's continued long term participation in the Deep Space Network


Attract and retain the best Australian students and staff in optics and photonics


Creation of photonics and space technology IP for commercial development


Take advantage of unique Australian capabilities

Australian technology becomes critical to deep space missions

Continued important role in space

FOR MORE INFO...

http://www.aao.gov.au/lasers


australian centre for space photonics andrew mcgrath anglo-australian observatory

Documents

exploration of mars

mars express

mars pathfinder

mars observer

mars odyssey slide

mars exploration rovers

planned mars exploration

mars reconnaissance