1
IAA-PDC17-05-19 The GOSSAMER Roadmap identified Multiple NEA Rendezvous as a science mission uniquely feasible only with solar sail propulsion. In addition, solar sailing also enables in-flight target change. The MASCOT lander technology enables asteroid surface access at instrument level of the carrier spacecraft. Both enable micro-class MNR missions. We welcome 2017 PDC ! EXERCISE – EXERCISE – EXERCISE – EXERCISE - EXERCISE EXERCISE – EXERCISE – EXERCISE – EXERCISE - EXERCISE EXERCISE – EXERCISE EXERCISE – EXERCISE The GOSOLAR project continues to develop common elements with the GOSSAMER solar sail deployment technology. The MASCOT project is developing a growing repertoire of lander designs through interest from small solar system body missions & studies. Together, they enable μ-MNR. the plan – Multiple NEA Rendezvous a trip to 5 NEAs for 100 days, each, in 10 years – Peloni, Ceriotti, Dachwald, 2016 – needs a c 0.2 mm/s² current GOSSAMER technology can do this – Seefeldt et al., 2016 – (50…70 m)² sail for 50…100 kg bus & payload a ~10 kg one-way asteroid lander is not just possible – Ho et al., 2016 – it’s flying! …and they do almost did another one …let’s go! sailcraft: GOSSAMER-1 technology by Seefeldt et al., 2016 11 kg with cradle 13 kg with radar passengers: MASCOT technology by Ho et al., 2016 35 kg with legs Soil to Sail – Asteroid Landers on Near-Term Sailcraft as an Evolution of the GOSSAMER Small Spacecraft Solar Sail Concept for In-Situ Characterization (1) DLR German Aerospace Center, Institute of Space Systems, Robert-Hooke-Strasse 7, 28359 Bremen, Germany – (2) +49-(0)421-24420-1107, [email protected] (3 )Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Solar Power Sail ISAS Pre-Project, 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa, 252-5210, Japan (4) University of Glasgow, Glasgow, Scotland G12 8QQ, United Kingdom (5) Faculty of Aerospace Engineering, FH Aachen University of Applied Sciences, Hohenstaufenallee 6, 52064 Aachen, Germany, +49-241-6009-52343 / -52854 (6) DLR German Aerospace Center, Robotics and Mechatronics Center, 82234 Wessling, Germany – (7) DLR German Aerospace Center, Institute of Planetary Research, Rutherfordstraße 2, 12489 Berlin, Germany (8) University of Colorado Boulder, 80309 Boulder, United States Jan Thimo Grundmann (1)(2) , Ralf Boden (3) , Matteo Ceriotti (4) , Bernd Dachwald (5) , Etienne Dumont (1) , Christian D. Grimm (1) , Caroline Lange (1) , Roy Lichtenheldt (6) , Ivanka Pelivan (7) , Alessandro Peloni (4) , Johannes Riemann (1) , Tom Spröwitz (1) , Simon Tardivel (8) Object Stay time [days] Start End Time of flight [days] Earth // 10 May 2025 26 Feb 2027 657 2000 SG 344 123 29 Jun 2027 06 Sep 2028 436 2015 JD 3 164 18 Feb 2029 24 Sep 2030 584 2012 KB 4 160 04 Mar 2031 29 Sep 2032 576 2008 EV 5 160 18 Mar 2033 22 May 2036 1161 Earth the extra mile: return to Earth extended from Peloni, Ceriotti, Dachwald, 2016 Object 2000 SG 344 2015 JD 3 2012 KB 4 2008 EV 5 2011 AG 5 Orbital type Aten Amor Amor Aten Apollo Semi-major axis [AU] 0.977 1.058 1.093 0.958 1.431 Eccentricity 0.067 0.009 0.061 0.083 0.390 Inclination [deg] 0.111 2.730 6.328 7.437 3.681 Absolute magnitude [mag] 24.7 25.6 25.3 20 21.8 Estimated size [m] 35 – 75 20 – 50 20 – 50 260 – 590 110– 240 EMOID [AU] 0.0008 0.054 0.073 0.014 0.0002 PHA no no no yes yes NHATS yes yes yes yes no Object Stay time [days] Start End Time of flight [days] Earth // 10 May 2025 26 Feb 2027 657 2000 SG 344 123 29 Jun 2027 06 Sep 2028 436 2015 JD 3 164 18 Feb 2029 24 Sep 2030 584 2012 KB 4 160 04 Mar 2031 29 Sep 2032 576 2008 EV 5 7.5 07 Oct 2032 25 May 2037 1691 2011 AG 5 987 to detour: 2011AG 5 – the PDC 2013 Exercise impactor imagined to hit on February 3 rd , 2040 extended from Peloni, Ceriotti, Dachwald, 2016 Object Stay time [days] Start End Time of flight [days] Earth // 13 Aug 2020 26 Apr 2022 621 2005 TG 50 128 02 Sep 2022 13 Jan 2024 498 2015 JF 11 104 25 Apr 2024 10 Jun 2026 776 2012 BB 14 139 28 Oct 2026 02 Aug 2028 644 2014 YN // Object 2017 PDC Semi-major axis [AU] 2.24 Eccentricity 0.607 Inclination [deg] 6.297 Right ascension of the ascending node [deg] 298 Argument of periapsis [deg] 312 Mean anomaly [deg] 332 Epoch [MJD] 57940 Absolute magnitude [mag] 21.9 Estimated size [m] 110 – 240 extended from Peloni, Ceriotti, Dachwald, 2016 chasing 2017 PDC – too little (a c celeration), too late (arrival) Exercise impactor imagined to hit on July 21 st , 2027 original sequence divert after 2 nd leg to fly to 2017 PDC 2017 PDC // 21 Aug 2030 >2000 (a c : 0.2 0.73 mm/s²) (1127 days = 3 years, 1 month after impact or close fly-by) one for all – all for one: get connected to the GOSSAMER principle of resource sharing in a 5-in-1 spacecraft – for example, power supply PHILAE heritage GOSSAMER–MASCOT co-developed umbilical connector, design based on reconstruction of PHILAE heritage BSDU CSCU HAYABUSA2 Remote Sensing Instruments Batt HPGP Science pg Batt chg sync Batt XFER Smplr / ldg gear Smplr / ldg gear container Remote Sensing Instruments Batt N2H4 Science pg Batt chg sync Batt XFER Smplr / ldg gear Smplr / ldg gear container Remote Sensing Instruments Remote Sensing Instruments Batt N2H4 Science pg Batt chg sync Batt XFER Smplr / ldg gear Smplr / ldg gear container Remote Sensing Instruments Remote Sensing Instruments Batt N2H4 Science pg Batt chg sync Batt XFER container Remote Sensing Instruments Remote Sensing Instruments SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER XFER Batt chg sync HPGP Science pg Batt Batt XFER container Remote Sensing Instruments Remote Sensing Instruments Batt chg sync HPGP Science pg Batt Batt XFER container Remote Sensing Instruments Remote Sensing Instruments Batt N2H4 Science pg Batt chg sync Batt XFER container Remote Sensing Instruments Remote Sensing Instruments SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt N2H4 Science pg Batt chg sync Batt XFER container Remote Sensing Instruments Remote Sensing Instruments SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt N2H4 Science pg Batt chg sync Batt XFER container Remote Sensing Instruments Remote Sensing Instruments SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt chg sync HPGP Science pg Batt Batt container Remote Sensing Instruments Remote Sensing Instruments XFER Batt N2H4 Science pg Batt chg sync Batt XFER container Remote Sensing Instruments Remote Sensing Instruments SURFACE N2H4 Science pg Batt Batt XFER SURFACE N2H4 Science pg Batt Batt XFER Batt chg sync XFER Remote Sensing Instruments Remote Sensing Instruments Batt chg sync XFER Remote Sensing Instruments Remote Sensing Instruments Batt chg sync HPGP Science pg Batt Batt XFER container Remote Sensing Instruments Remote Sensing Instruments Batt chg sync HPGP Science pg Batt Batt XFER container Remote Sensing Instruments Remote Sensing Instruments Batt chg sync HPGP Science pg Batt Batt XFER container Remote Sensing Instruments Remote Sensing Instruments Batt chg sync HPGP Science pg Batt Batt XFER Remote Sensing Instruments Remote Sensing Instruments Batt chg sync XFER Remote Sensing Instruments Remote Sensing Instruments Batt chg sync XFER Remote Sensing Instruments Remote Sensing Instruments Batt chg sync Remote Sensing Instruments Remote Sensing Instruments Batt chg sync Remote Sensing Instruments Remote Sensing Instruments XFER XFER XFER XFER XFER XFER HPGP Science pg Batt Batt HPGP Science pg Batt Batt HPGP Science pg Batt Batt HPGP Science pg Batt Batt a few kg … 100 kg 500 kg 250 kg 50 kg kickstart: small sail, big launcher modelled performance of the Ariane 5 ECA with very small payoads: 50 kg: minimum MASCOT-like flyby spacecraft or NEASCOUT(s) 250 kg: Multiple NEA Rendezvous (1-way) or DEEP IMPACT Bus reflight 500 kg: dual MNR (1-way) or NEW HORIZONS,HAYABUSA2 reflight extended from Dumont & David., 2013 Object Stay time [days] Start End Time of flight [days] Earth // 10 May 2025 26 Feb 2027 657 2000 SG 344 123 29 Jun 2027 06 Sep 2028 436 2015 JD 3 164 18 Feb 2029 24 Sep 2030 584 2012 KB 4 160 04 Mar 2031 29 Sep 2032 576 2008 EV 5 171 20 Mar 2033 30 Sep 2034 560 2014 MP // Object Earth 2000 SG 344 2015 JD 3 2012 KB 4 2008 EV 5 2014 MP Orbital type - Aten Amor Amor Aten Amor Semi-major axis [AU] 1 0.977 1.058 1.093 0.958 1.050 Eccentricity 0 0.067 0.009 0.061 0.083 0.029 Inclination [deg] 0 0.111 2.730 6.328 7.437 9.563 Absolute magnitude [mag] - 24.7 25.6 25.3 20 26 Estimated size [m] - 35 – 75 20 – 50 20 – 50 260 – 590 17 – 37 EMOID [AU] - 0.0008 0.054 0.073 0.014 0.020 PHA - no no no yes no NHATS - yes yes yes yes yes itinerary: considered sequence of Peloni, Ceriotti, Dachwald, 2016 2008 EV 5 2014 MP 2000 SG 344 2000 SG 344 2000 SG 344 2000 SG 344 2015 JD 3 2015 JD 3 2015 JD 3 2015 JD 3 2012 KB 4 2012 KB 4 2012 KB 4 2012 KB 4 2008 EV 5 2008 EV 5 2008 EV 5 2008 EV 5 2014 MP 2014 MP 2014 MP 2014 MP Batt chg sync Remote Sensing Instruments Remote Sensing Instruments Batt chg sync Remote Sensing Instruments Remote Sensing Instruments

Soil to Sail – Asteroid Landers on Near-Term Sailcraft as an …elib.dlr.de/118805/3/IAA-PDC-17-05-19po.pdf · 2018-02-06 · Object 2000 SG344 2015 JD3 2012 KB4 2008 EV5 2011 AG5

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IAA-PDC17-05-19

The GOSSAMER Roadmap identified Multiple NEA Rendezvous as a science mission uniquely feasible only with solar sail propulsion. In addition, solar sailing also enables in-flight target change. The

MASCOT lander technology enables asteroid surface access at instrument level of the carrier

spacecraft. Both enable micro-class MNR missions.

We welcome 2017 PDC !

EXERCISE – EXERCISE – EXERCISE – EXERCISE - EXERCISE

EXERCISE – EXERCISE – EXERCISE – EXERCISE - EXERCISE

EXER

CISE –

EXER

CISEEX

ERC

ISE

–EX

ERC

ISE The GOSOLAR project continues to develop common elements with the GOSSAMER solar sail

deployment technology. The MASCOT project is developing a growing repertoire of lander designsthrough interest from small solar system body missions & studies. Together, they enable μ-MNR.

the plan – Multiple NEA Rendezvous① a trip to 5 NEAs for 100 days, each, in 10 years – Peloni, Ceriotti, Dachwald, 2016 – needs ac ≥ 0.2 mm/s²② current GOSSAMER technology can do this – Seefeldt et al., 2016 – (50…70 m)² sail for 50…100 kg bus & payload③ a ~10 kg one-way asteroid lander is not just possible – Ho et al., 2016 – it’s flying! …and they do almost did another one

…let’s go!

sailcraft: GOSSAMER-1 technology by Seefeldt et al., 2016

11 kg with cradle 13 kg with radar

passengers: MASCOT technology by Ho et al., 2016

35 kg with legs

Soil to Sail – Asteroid Landers on Near-Term Sailcraftas an Evolution of the GOSSAMER Small Spacecraft

Solar Sail Concept for In-Situ Characterization

(1)DLR German Aerospace Center, Institute of Space Systems, Robert-Hooke-Strasse 7, 28359 Bremen, Germany – (2)+49-(0)421-24420-1107, [email protected](3)Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), Solar Power Sail ISAS Pre-Project, 3-1-1 Yoshinodai, Chuo, Sagamihara, Kanagawa, 252-5210, Japan

(4)University of Glasgow, Glasgow, Scotland G12 8QQ, United Kingdom (5)Faculty of Aerospace Engineering, FH Aachen University of Applied Sciences, Hohenstaufenallee 6, 52064 Aachen, Germany, +49-241-6009-52343 / -52854

(6)DLR German Aerospace Center, Robotics and Mechatronics Center, 82234 Wessling, Germany – (7)DLR German Aerospace Center, Institute of Planetary Research, Rutherfordstraße 2, 12489 Berlin, Germany (8)University of Colorado Boulder, 80309 Boulder, United States

Jan Thimo Grundmann(1)(2), Ralf Boden(3), Matteo Ceriotti(4), Bernd Dachwald(5), Etienne Dumont(1), Christian D. Grimm(1), Caroline Lange(1), Roy Lichtenheldt(6), Ivanka Pelivan(7), Alessandro Peloni(4),

Johannes Riemann(1), Tom Spröwitz(1), Simon Tardivel(8)

Object Stay time

[days] Start End

Time of flight [days]

Earth //

10 May 2025 26 Feb 2027 657 2000 SG344 123

29 Jun 2027 06 Sep 2028 436

2015 JD3 164

18 Feb 2029 24 Sep 2030 584

2012 KB4 160

04 Mar 2031 29 Sep 2032 576

2008 EV5 160

18 Mar 2033 22 May 2036 1161

Earth ∞

the extra mile: return to Earth

extended from Peloni, Ceriotti, Dachwald, 2016

Object 2000 SG344 2015 JD3 2012 KB4 2008 EV5 2011 AG5

Orbital type Aten Amor Amor Aten Apollo

Semi-major axis [AU] 0.977 1.058 1.093 0.958 1.431

Eccentricity 0.067 0.009 0.061 0.083 0.390

Inclination [deg] 0.111 2.730 6.328 7.437 3.681 Absolute magnitude [mag]

24.7 25.6 25.3 20 21.8

Estimated size [m] 35 – 75 20 – 50 20 – 50 260 – 590 110– 240

EMOID [AU] 0.0008 0.054 0.073 0.014 0.0002

PHA no no no yes yes

NHATS yes yes yes yes no

Object Stay time

[days]

Start End Time of flight

[days] Earth //

10 May 2025 26 Feb 2027 657 2000 SG344

123

29 Jun 2027 06 Sep 2028

436 2015 JD3 164

18 Feb 2029 24 Sep 2030

584 2012 KB4 160

04 Mar 2031 29 Sep 2032

576 2008 EV5 7.5

07 Oct 2032 25 May 2037

1691 2011 AG5 987 to ⊕

detour: 2011AG5 – the PDC 2013 Exercise impactor imagined to hit on February 3rd, 2040

extended from Peloni, Ceriotti, Dachwald, 2016

Object Stay time

[days]

Start End Time of flight

[days] Earth //

13 Aug 2020 26 Apr 2022 621 2005 TG50 128

02 Sep 2022 13 Jan 2024 498 2015 JF11 104

25 Apr 2024 10 Jun 2026 776 2012 BB14 139

28 Oct 2026 02 Aug 2028 644 2014 YN //

Object 2017 PDC

Semi-major axis [AU] 2.24

Eccentricity 0.607

Inclination [deg] 6.297

Right ascension of the ascending node [deg] 298

Argument of periapsis [deg] 312

Mean anomaly [deg] 332

Epoch [MJD] 57940

Absolute magnitude [mag] 21.9

Estimated size [m] 110 – 240

extended from Peloni, Ceriotti, Dachwald, 2016

chasing 2017 PDC – too little (acceleration), too late (arrival)Exercise impactor imagined to hit on July 21st, 2027

original sequence

divert after 2nd leg to fly to 2017 PDC

2017 PDC // 21 Aug 2030 >2000(ac: 0.2 0.73 mm/s²)

(1127 days = 3 years, 1 month after impact or close fly-by)

one for all – all for one: get connected to the GOSSAMER principle ofresource sharing in a 5-in-1 spacecraft – for example, power supply

PHILAE heritage

GOSSAMER–MASCOT co-developedumbilical connector, design based on reconstruction of PHILAE heritage

BSDU CSCUHAYABUSA2

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a few kg … ≈100 kg

500 kg250 kg

50 kg

kickstart: small sail, big launcher

modelled performance of the Ariane 5 ECA with very small payoads:50 kg: minimum MASCOT-like flyby spacecraft or NEASCOUT(s)

250 kg: Multiple NEA Rendezvous (1-way) or DEEP IMPACT Bus reflight500 kg: dual MNR (1-way) or NEW HORIZONS, HAYABUSA2 reflight

extended from Dumont & David., 2013

Object Stay time

[days]

Start End Time of flight

[days] Earth //

10 May 2025 26 Feb 2027 657

2000 SG344 123

29 Jun 2027 06 Sep 2028 436

2015 JD3 164

18 Feb 2029 24 Sep 2030 584

2012 KB4 160

04 Mar 2031 29 Sep 2032 576

2008 EV5 171

20 Mar 2033 30 Sep 2034 560

2014 MP // Object Earth 2000 SG344 2015 JD3 2012 KB4 2008 EV5 2014 MP

Orbital type - Aten Amor Amor Aten Amor

Semi-major axis [AU] 1 0.977 1.058 1.093 0.958 1.050

Eccentricity 0 0.067 0.009 0.061 0.083 0.029

Inclination [deg] 0 0.111 2.730 6.328 7.437 9.563

Absolute magnitude [mag]

- 24.7 25.6 25.3 20 26

Estimated size [m] - 35 – 75 20 – 50 20 – 50 260 – 590 17 – 37

EMOID [AU] - 0.0008 0.054 0.073 0.014 0.020

PHA - no no no yes no

NHATS - yes yes yes yes yes

itinerary: considered sequence of Peloni, Ceriotti, Dachwald, 2016

2008 EV5

2014 MP

2000 SG3442000 SG344

2000 SG344

2000 SG344

2015 JD3

2015 JD3 2015 JD3

2015 JD3

2012 KB4

2012 KB4

2012 KB4

2012 KB4

2008 EV5

2008 EV5

2008 EV5

2008 EV5

2014 MP

2014 MP

2014 MP

2014 MP

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