Scientific Mission Applications

Slides:



Advertisements
Similar presentations
The BepiColombo Mission
Advertisements

ASTR1001: Mountains and Atmospheres. Summary In this section, we will talk about the mountains of different planets, and about their atmospheres. Puzzle.
Gravitational Potential Energy When we are close to the surface of the Earth we use the constant value of g. If we are at some altitude above the surface.
Low-thrust trajectory design ASEN5050 Astrodynamics Jon Herman.
Mission To Mars In Kerbal Space Program, Where distances are 1/9 real world values.
1 Interstellar Heliopause Probe M. Leipold, Kayser-Threde GmbHISSS 2010, New York, July 19 – 22, 2010 Interstellar Heliopause Probe (IHP) System Design.
1 ESAIL proof of concept mission Juha-Pekka Luntama Pekka Janhunen Petri Toivanen.
SATELLITES What They Do and How They Work Michael J. Mackowski Aerospace Engineer October 2013 With Updates from Shawn Shepherd.
EGR 4347 Analysis and Design of Propulsion Systems
Spacecraft Propulsion Dr Andrew Ketsdever Lesson 13 MAE 5595.
Solar system science using X-Rays Magnetosheath dynamics Shock – shock interactions Auroral X-ray emissions Solar X-rays Comets Other planets Not discussed.
1 Possibilities for Traveling to Mars Charles C. Renn.
Gravitational Potential Energy When we are close to the surface of the Earth we use the constant value of g. If we are at some altitude above the surface.
Today’s APODAPOD  Read NASA website:  solarsystem.nasa.gov solarsystem.nasa.gov  IN-CLASS QUIZ THIS FRIDAY!!  Solar Lab, Kirkwood, Rooftop this week.
“ PHOBOS - SOIL ” Phobos Sample Return Mission 1. goals, methods of study A.Zakharov, Russian academy of sciences Russian aviation.
Optimal Low-Thrust Deorbiting of Passively Stabilized LEO Satellites Sergey Trofimov Keldysh Institute of Applied Mathematics, RAS Moscow Institute of.
Titan Mariner Spacecraft Study Titan Team! IPPW-5 June 24, 2007.
Spacecraft Instruments. ► Spacecraft instrument selection begins with the mission description and the selected primary and secondary mission objectives.
The Sun and the Heliosphere: some basic concepts…
Bob G. Beaman June 28, 2001 Electrical Power System SuperNova / Acceleration Probe (SNAP)
The Sun. Solar Prominence Sun Fact Sheet The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. Diameter: 1,390,000 km (Earth.
Computer Simulations in Solar System Physics Mats Holmström Swedish Institute of Space Physics (IRF) Forskarskolan i rymdteknik Göteborg 12 September 2005.
Uranus and Neptune Uranus: general information –Discovered in 1781 (Herschel) –Radius about 4x that of Earth –Mass about 14.5x that of Earth –Nearly featureless.
EXTROVERTSpace Propulsion 02 1 Thrust, Rocket Equation, Specific Impulse, Mass Ratio.
February 18, 2006HYPERION ERAU 1 Interstellar Travel Now.
Electric Sail Technology Status Review Pekka Janhunen Finnish Meteorological Institute, (Kumpula Space Centre) ESA/ESTEC May 19, 2008.
Bits and Pieces. Spacecraft Systems Propulsion –Already discussed Communications Science instruments Power.
 The Venus Express Mission Håkan Svedhem Project Scientist ESAC, Spain 27 April 2010.
Dawn Dawn Mission. Dawn How Do We Get There? Dawn DAWN A Journey to the Beginning of the Solar System Vesta Travel Plans: Dawn’s Itinerary The Dawn Spacecraft.
PLANETARY PROBE LASER PROPULSION CONCEPT 7 TH INTERNATIONAL PLANETARY PROBE WORKSHOP JUNE 2009, BARCELONA LE, T. (1), MOBILIA, S. (2), PAPADOPOULOS,
29 Sept 03Solar System - Dr. C.C. Lang1 Exploring the Solar System: all about spacecraft/spaceflight.
Spacecraft Trajectories You Can Get There from Here! John F Santarius Lecture 9 Resources from Space NEEP 533/ Geology 533 / Astronomy 533 / EMA 601 University.
MYSTERIES OF EARTH AND MARS Unit One Physical Science (or, getting there from here) An Overview By - Jack Forristel -
Introduction to Space Weather Jie Zhang CSI 662 / PHYS 660 Spring, 2012 Copyright © The Heliosphere: The Solar Wind March 01, 2012.
The Dangers of Solar Storms and Solar Cycles.  Radius = 696,000 km  Mass = 2E30 kg  Luminosity = 3.8E26 W  Rotation Rate  25 days at the equator.
Exploring the Solar System: all about spacecraft/spaceflight
FAST LOW THRUST TRAJECTORIES FOR THE EXPLORATION OF THE SOLAR SYSTEM
1 Grades 6-8: Introduction. 2 Aerospace Technology Space Science Human Exploration And Development Of Space Earth Science Main Areas Of Research.
CRRES observations indicate an abrupt increase in radiation belt fluxes corresponding to the arrival of a solar wind shock. The processes(s) which accelerate.
The Suprathermal Tail Properties are not well understood; known contributors Heated solar wind Interstellar and inner source pickup ions Prior solar and.
ERAU Space Physics Program1 Space Physics Program College of Arts & Sciences ERAU-Prescott Dr. Darrel Smith World Space Congress October 17, 2002.
Exploring 16 Psyche: Psyche Orbiter
The Sun. Sun Fact Sheet The Sun is a normal G2 star, one of more than 100 billion stars in our galaxy. Diameter: 1,390,000 km (Earth 12,742 km or nearly.
Goal to understand how Ion Propulsion works.
Saturn In many ways, Saturn resembles a smaller version of Jupiter
The Future of Human Spaceflight *** A Journey to Mars
The Giant Planets Beyond Mars and the asteroids are the giant or Jovian planets Jupiter, Saturn, Uranus, Neptune Pluto is part of the outer solar system.
Cost Comparison of Higher Parking Orbit Scale up for Arbitrary Payload
CRCT Preparation.
Solar Probe Plus Scheduled to be launched in 2018 Solar Probe Plus will come closer to the Sun than any spacecraft has ever flown - and what it finds could.
Goal to understand how Solar Sails work.
Lecture on Spacecraft / Spaceflight
Technical Resource Allocations
A Parametric Study of Interplanetary Mission Using Solar Sail
Properties of the Atmosphere
An Introduction to the Upper Atmosphere
Mozella Bell, Herman Neal, Matthew Ware
PROJECT METEOR: RITSAT1 P08102
Bellwork 12/22 What kinds of design differences would there be in planning a mission to Jupiter versus sending a satellite into Earth’s orbit?
NASA NASA's Parker Solar Probe mission set off to explore the Sun's atmosphere on Sunday morning August 12, It will swoop to within 4 million miles.
Solar Activity and Space Weather
Goal to understand how Ion Propulsion works.
Bellwork 1/8 What do you know about the International Space Station? If you could ask someone living on the International Space Station some questions,
The Sun.
Classroom Rocket Scientist
Grades 9-12: Introduction
The Ionosphere Equatorial Anomaly.
The Sun.
Planet Earth.
CHEOPS - CHaracterizing ExOPlanet Satellite
Presentation transcript:

Scientific Mission Applications P. K. Toivanen, P. Janhunen, and J.-P. Luntama 22.9.2018

Outline Example mission to Mars Optimal orbit to Mars Optimal operation of the sail Optimal operations and real solar wind Solar wind variations and sail performance Density variations Wind speed variations Average performance Tether voltage and navigation Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Electric sail and science missions About mass budget of electric sail About economics of electric sail missions Interstellar Heliospheric Probe (IHP) Kuiper/centaur flyby mission Asteroid tour Space weather monitoring Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Optimal orbit to Mars Mengali, Quarta, and Janhunen: Journal of Spacecraft and Rockets, 2008. Solar wind speed, 400 km/s Density, 7.3 cm-3 Electron temperature,12 eV Radial scaling laws for the solar wind parameters Total mass 200 kg Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Optimal operation of the sail Optimal solution includes: Initial acceleration of about 0.5 mm/s2 (Earth) Coasting phase (shading) Constant thrust angle of 20 deg Acceleration at Mars of about 0.3 mm/s2 Travel time of 600 days Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Optimal operations and real solar wind Varying density and speed: Acceleration varies about 40% around the average Mars missed! But s/c kind of got there… Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Solar wind variations and sail performance Some severe weather conditions: Densities higher than 30 cm-3 may occur Solar wind speed may be higher than 1000 km/s Variations in acceleration far more mellow than those of the solar wind driving the sail Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Density variations Acceleration limited: Electron current to the tethers increases Electron gun power limited by the given solar panel power Tether voltage drops Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Wind speed variations #1 Acceleration is regulated: Solar wind speed drive not linear: Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Wind speed variations #2 For small wind speed values: Solar wind kinetic energy less than the tether electric potential Dynamic pressure term dominates For large wind speed values: Solar wind kinetic energy larger than the tether electric potential Solar wind penetrates to the tether potential structure Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Average performance #1 3-month averaged thrust in cases of: Limited tether voltage (40 kV, thick) No tether voltage limitation (thin) Variations relatively small around average at 70 nN/m Missions can be desinged for the minimum thrust (dotted) without missing much of the maximum thrust (dashed) Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Average performance #2 Thrust vs. solar panel power: For small power values, difference between the maximum and minimum thrust not large For large power values, the minimum thrust saturates Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Average performance #3 Thrust vs. averaging window: Down to averaging over about ten days, difference between maximum and minimum thrust does not change dramatically Averages below ten days are not relevant in mission time scales Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Tether voltage and navigation Simple navigation procedure: Onboard accelerometer Time-integrate measured acceleration for spacecraft speed, Vsc Compare hourly Vsc with speed at optimal orbit, V0 If Vsc < V0, increase tether potential by 5kV for the next hour If Vsc > V0, decrease tether potential by 5kV for the next hour Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Electric sail and science missions High delta-v for small payloads Interplanetary Heliospheric Probe (IHP) Kuiper/Centaur flyby mission Asteroid tour Space weather monitoring Other missions Near-solar missions Planetary missions Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Electric sail propulsion system 100 X 20 km aluminium four-fold Hoytether Tethers: 7.3 kg (20 µm) Reels: 22.0 kg (3 X tethers) Electron gun + radiator: 1.5 kg (40 kV & 1kW) High-voltage power source: 2.0 kg Avionics + tether direction sensor: 7.0 kg Solar panels: 6.0 kg (1.1 kW) Battery Li-ion: 1.0 kg (8 Ah) S/c frame with thermal isolation: 4.5 kg AOCS thrusters: 1.0 kg Total: 52.3 kg Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

About economics of electric sail missions Payload more expensive than the launch Soyuz-fregat: 1.3 ton payload to escape orbit Electric sailer with 1.3 ton payload accelerates slowly Smaller booster saves no that much 4-6 electric sailers per launch Piggybag Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Interstellar Heliospheric Probe Fast flight to interstellar medium: Formation of the heliosphere Pioneer anomaly Present proposed mission time is tens of years Electric sailer is an enabling technology Reduced travel time Weight issue Use of several electric sailers Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Kuiper/centaur flyby mission Properties of primoidal objects: Group of flyby probes, target per probe One launch with Siamise Twins spin-up for each pair Small payload (total mass 150-200 kg) Minimal instrument set only to study the target Fast travel time Fast flyby, data into memory and slow downloading Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Asteroid tour More for the same money: Single electric sailer can visit several asteroids Water/hydrogen on asteroids Mineral composition Morphology Imager, radar, and spectroscope (infrared, neutron, and gamma) Shoot bullet with a railgun Laser heating Micrometeor flashes on dark side Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018

Space weather monitoring Off-Lagrange point monitoring: Propellantless operation needed Longer than the 1-hour time delay to Earth (solar wind) Solar wind monitoring for other planet missions (as a piggybag) Tether voltage cycled: off during monitoring on during orbit control Ilmatieteen laitos / PowerPoint ohjeistus 22.9.2018