spaceup stuttgart 2012 - ruediger jehn mercury is challenging us

14
R. Jehn | ESA/ESOC | 14 September 2012 | Page 1 HSO-GFA- Mission Analysis Section What is wrong with Mercury? Rüdiger Jehn European Space Operations Centre/ European Space Agency

Upload: aerospaceresearch

Post on 06-Aug-2015

49 views

Category:

Documents


1 download

DESCRIPTION

Slides of the SpaceUp Stuttgart 20 minutes talk by Ruediger Jehn

TRANSCRIPT

What is wrong with Mercury?Rdiger JehnEuropean Space Operations Centre/ European Space Agency

R. Jehn | ESA/ESOC | 14 September 2012 | Page 1 HSO-GFA- Mission Analysis Section

Mercury still is a challenge! Diameter: 4880 km (38 % of the Earth, 140 % of the Moon) Distance to Sun: 46 - 70 million km (0.39 AU)

Images courtesy of NASA

R. Jehn | ESA/ESOC | 14 September 2012 | Page 2 HSO-GFA- Mission Analysis Section

Early Deceptions1881-1889 Giovanni SchiaparelliRotation rate: 88 days

1896-1897 Percival Lowell

R. Jehn | ESA/ESOC | 14 September 2012 | Page 3 HSO-GFA- Mission Analysis Section

From Das unendliche Weltall Grundlagen der Astronomie (1966):

R. Jehn | ESA/ESOC | 14 September 2012 | Page 4 HSO-GFA- Mission Analysis Section

The truth

1965 Arecibo radio telescope

Rotation rate:58.65 days !

R. Jehn | ESA/ESOC | 14 September 2012 | Page 5 HSO-GFA- Mission Analysis Section

Sunrise on Mercury

click to start the Sun rise on Mercury

R. Jehn | ESA/ESOC | 14 September 2012 | Page 6 HSO-GFA- Mission Analysis Section

Pear shape of Mercury: J3

R. Jehn | ESA/ESOC | 14 September 2012 | Page 7 HSO-GFA- Mission Analysis Section

Spy at AGU Dec 2011 in San Francisco

R. Jehn | ESA/ESOC | 14 September 2012 | Page 8 HSO-GFA- Mission Analysis Section

Mercury: Solid or Liquid Core?

Radar observations presented in July 2004 in ParisLibration Amplitude: 60 arcsec

R. Jehn | ESA/ESOC | 14 September 2012 | Page 9 HSO-GFA- Mission Analysis Section

Libration of MercuryPublication in Science, Vol 316, 4 May 2007:

R. Jehn | ESA/ESOC | 14 September 2012 | Page 10 HSO-GFA- Mission Analysis Section

High Density

R. Jehn | ESA/ESOC | 14 September 2012 | Page 11 HSO-GFA- Mission Analysis Section

High Density1. Crust: 100300 km thick 2. Mantle: 600 km thick 3. Core: 1,800 km radius

3 Theories for Mercurys Origin:

1. Selective Accretion (SA) 2. Post-accretion Vaporisation (V) 3. Giant Impact (GI)R. Jehn | ESA/ESOC | 14 September 2012 | Page 12 HSO-GFA- Mission Analysis Section

Way aheadBepiColombo Launch: 16 August 2015 Arrival at Mercury: 27 Jan 2022 500 kg Xenon for ionpropulsion MMO (Jaxa): 400 x 12000 km MPO (ESA): 400 x 1500 kmR. Jehn | ESA/ESOC | 14 September 2012 | Page 13 HSO-GFA- Mission Analysis Section

BepiColombo

Challenges to explore Mercury 7 flybys Spacecraft often behind the Sun Ion-propulsion unit Solar arrays get too hot Thermal protection against 11 Suns

R. Jehn | ESA/ESOC | 14 September 2012 | Page 14 ESA UNCLASSIFIED -- For Official Use

HSO-GFA- Mission Analysis Section