/
PLANETARY EXPLORATION!!! PLANETARY EXPLORATION!!!

PLANETARY EXPLORATION!!! - PowerPoint Presentation

pamella-moone
pamella-moone . @pamella-moone
Follow
406 views
Uploaded On 2016-06-18

PLANETARY EXPLORATION!!! - PPT Presentation

Logan Dougherty Quick Overview Mariner 2 First successful Venus flyby USA Mariner 4 First successful Mars flyby USA Venera 3 First Venus impact Contact lost USSR Venera 4 Venus atmospheric probe ID: 367178

mars planetary mission science planetary mars science mission solar missions system planets http amp discovery budget life launch program

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "PLANETARY EXPLORATION!!!" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

PLANETARY EXPLORATION!!!

Logan DoughertySlide2

Quick OverviewMariner 2 – First successful Venus flyby (USA)Mariner 4 – First successful Mars flyby (USA)

Venera 3 – First Venus impact. Contact lost. (USSR)Venera 4 – Venus atmospheric probeClaimed to reach the surface intact, but disproven shortly after by USA Mariner 5.

Pioneer 10 & 11 – Jupiter and Saturn flyby

Mariner 10 – Mercury flyby

Voyager 1 & 2 – Outer solar system

Pathfinder – Mars rover

Cassini Huygens – Saturn lander

New Horizons – Pluto and Kuiper belt

Curiosity

Rover – Mars RoverSlide3

Above: To the left is the Mariner 2 and

to the right is the Voyager 1.

Right: The New Horizons spacecraft.Slide4

Original Reasons for Planetary ExplorationThe Space RaceMain memorable part of the Space Race is the Apollo missionLarge competition in planetary exploration as well

Between USA and USSRhttp://nssdc.gsfc.nasa.gov/planetary/chronology.htmlAs shown above, until the end of the Cold War, USA and USSR competed largely in their attempts to study the moon and the planets.

Post Cold War, the USSR involvement declined heavily, leaving the USA to dominate the fieldSlide5
Slide6

NASA’s Big Questions for Planetary ScienceHow did the sun's family of planets and minor bodies originate?

How did the solar system evolve to its current diverse state?How did life begin and evolve on Earth, and has it evolved elsewhere in the Solar System?

What are the characteristics of the Solar System that lead to the origins of life?Slide7

President’s FY13 In-Guide Budget

For FY13 Congress has passed a “Continuing Resolution”

Under the CR PSD’s FY13 budget is $1.19B

21% decrease from FY12 levelSlide8

Amazing AccomplishmentsExistence of bodies of water on Mars in the past.Atmospheric probes to help determine composition of other planets.Missions that help deduce the early evolution of planets and help to explain why our solar system formed how it did.

Valuable samples of surfaces that offer insight into the formation of that planet.Slide9

What inspires Planetary Exploration?Slide10

Search for Life near HomeMarsSigns of water, as discovered by rovers like CuriosityVenusPeople used to envision life existing there, but the harsh atmosphere makes it difficult to support life

TitanLiquid lakes of ethane and methaneColder than earthAtmosphere that consists of more than trace gasesSlide11

Where else should we search?Slide12

Exoplanet DetectionKepler missionUses transit method to detect dip in light curvesDoppler Shift measurements

Binary MovementsHundreds of planets have been discoveredPlanetary Detection is part of the Astrophysics sector of NASA as opposed to the Planetary Science, but offers useful information in the theory of how solar systems evolve.Exoplanets are popular

The idea inspires people and the public is interested in the possibility of finding planets with lifeSlide13

What is the biggest difficulty in directly observing a planet?Slide14
Slide15

New WorldsBlocks out the star’s light to gain a direct view of the planet.Can then study the spectra of the planet and gain knowledge of its atmosphere.Offers the possibility of finding planets capable of hosting life

Reasons that policy makers may consider investing:While Kepler has produced results, the public keeps hearing about planets and it doesn’t peak their interest.

This would offer a more definitive statement on the possibility of life, and to see more detailed pictures of the planets, garnering more public support.

Offers useful knowledge about planet’s in the habitable zone of stars.Slide16

“Space: the final frontier.”Slide17

Works Citedhttp://www.newscientist.com/data/images/archive/2542/25424001.jpg

http://cinema-wallpapers.net/user-content/uploads/wall/o/60/Little-Green-Men-toy-story-2-wallpaper.jpghttp://jpl.nasa.gov

http://science.nasa.gov/planetary-science

/

http://

ut-images.s3.amazonaws.com/wp-content/uploads/2011/02/Kepler-telescope.jpg

http://4.bp.blogspot.com/_

FQaCDdht2S8/TEybVhkHILI/AAAAAAAABDc/wi6q8fMoElo/s1600/newhorizons.gifhttp://

ut-images.s3.amazonaws.com/wp-content/uploads/2008/07/voyager1.jpg

http://

www.nasa.gov/images/content/203286main_image_964_946-710.jpg

http://

iliketowastemytime.com/system/files/outer-space-hd-wallpaper.jpg?download=1

http://

i.telegraph.co.uk/multimedia/archive/02445/AV_2445412b.jpgSlide18

NASA

s Planetary Science Division

James L. Green

Director, Planetary Science Division

NASA Headquarters

February 21, 2013Slide19

Recent Accomplishments

2010

* September 16 – Lunar Reconnaissance Orbiter in PSD

* November 4 - EPOXI encounters Comet Hartley 2

* November 19 - Launch of O/OREOS

2011

* February 14 - Stardust NExT encounters comet Tempel 1

* March 7 – Planetary Science Decadal Survey released

* March 17 - MESSENGER orbit insertion at Mercury

* May 5 – Selection of 3 Discovery-class missions for study

* May – Selection of the next New Frontier mission for flight, OSIRIS-REx

* July 16 - Dawn orbit insertion at asteroid Vesta

* August 5 - Juno launch to Jupiter

* August 9 - Mars Opportunity Rover arrives at Endeavour Crater

* September 10 - GRAIL (A and B) launch to the Earth

s Moon

* November 26 – Mars Science Laboratory (MSL) launch to Mars

* December 31 – GRAIL A orbit insertion at Earth

s Moon

2012

* January 1 – GRAIL B orbit insertion at Earth

s Moon

* June 6 – Venus transits Sun (last time this Century)

* August 5 – MSL/Curiosity successfully lands on Mars

* August 20 – Selection of Discovery 12 Mission

* September 5 - Dawn leaves Vesta and starts on its journey to Ceres

*

CompletedSlide20

The Revolution in

Planetary Science

20

Planetary Decadal Reports from the

National Academy of Science Slide21

Planetary Science ObjectivesNASA

’s goal in Planetary Science is to “

Ascertain the content, origin, and evolution of the solar system, and the potential for life elsewhere

.

Planetary Program

seeks to answer fundamental science questions:

What is the inventory of solar system objects and what processes are active in and among them?

How did the Sun

s family of planets, satellites, and minor bodies originate and evolve?

What are the characteristics of the solar system that lead to habitable environments?

How and where could life begin and evolve in the solar system?

What are characteristics of small bodies and planetary environments that pose hazards and/or provide resources?

21

Planetary Science accomplishes these goals through a series of

strategic-large, medium, small mission and supporting research Slide22

Planetary Decadal Recommendations

22

Technology Development (6-8%)

Research & Analysis (5% above final FY11 amount then ~1.5%/yr)

Discovery

$500M (FY15) cap per mission (exclusive of launch vehicle) and 24 month cadence for selection

New Frontiers

$1B (FY15) cap per mission (exclusive of launch vehicle) with two selections during 2013-22

Large Missions (

Flagship

-scale)

Recommended Program

(budget increase for JEO new start)

Mars Astrobiology Explorer-Cacher – descoped

Jupiter Europa Orbiter (JEO) – descoped

Uranus Orbiter & Probe (UOP

)

4/5) Enceladus Orbiter & Venus Climate Mission

Cost Constrained Program

(based on FY11 Request)

Mars Astrobiology Explorer-Cacher – descoped

Uranus Orbiter & Probe (UOP)

Less favorable

budget picture than assumed

(e.g., outyears in FY12 request)

Descope or delay Flagship mission

Current Commitments (

ie: Operating Missions

)Slide23

President’s FY13 In-Guide Budget

For FY13 Congress has passed a “

Continuing Resolution

Under the CR PSD

s FY13 budget is $1.19B21% decrease from FY12 levelSlide24

Planetary & President’s FY13 Budgets Slide25

President’s FY13 Budget - Missions

Mars

R&A

Discovery

New Frontiers

Technology

Outer Planets

Mars 2020

MAVEN

OSIRIS-REx

InSight

LADEESlide26

Discovery and New Frontiers

Address high-priority science objectives in solar system exploration

Frequent opportunities for science community to propose full investigations

Fixed-price cost cap full and open competition missions

Principal Investigator-led project

Established in 1992

$425M cap

per mission excluding launch vehicle (FY10)

Open science competition for all solar system objects, except for the Earth and Sun

Established in 2003

$1000M

cap per mission excluding launch vehicle (FY10)

Addresses high-priority investigations identified by the National Academy of SciencesSlide27

27

Discovery Program

Mars evolution:

Mars Pathfinder (1996-1997)

NEO characteristics:

NEAR (1996-1999)

Lunar formation:

Lunar Prospector (1998-1999)

Completed

Comet internal structure:

Deep Impact (2005-2012)

Mercury environment:

MESSENGER (2004

-

2013

)

Main-belt asteroids: Dawn (

2007-2015

)

Lunar Internal Structure

GRAIL (

2011-2012

)

In Flight

Comet diversity:

CONTOUR

Solar wind sampling:

Genesis (2001-2004)

Nature of dust/coma:

Stardust (1999-2011 )

Lost

Aug 15 2002

CompletedSlide28

InSight: Interior Structure from Seismic Investigations, Geodesy and Heat Transport

28Slide29

New Frontiers Program

1

st

NF mission

New Horizons:

Pluto-Kuiper Belt

Launched January 2006

Arrives July 2015

PI: Alan Stern (SwRI-CO)

2

nd

NF mission

JUNO:

Jupiter Polar Orbiter

3

rd

NF mission

OSIRIS-REx

Launched August 2011

Arrives July 2016

PI: Scott Bolton (SwRI-TX)

Asteroid Sample Return

Sept. 2016 LRD

PI: Dante Lauretta (UA)

NF-4 AO in FY15-16Slide30

O

rigins-

S

pectral

I

nterpretation-

R

esource

I

dentification-

S

ecurity-

R

egolith

Ex

plorer (OSIRIS-REx )

Science Objectives:

Return and analyze a sample of pristine carbonaceous asteroid

Map the global properties, chemistry, and mineralogy

Document in situ the properties of the regolith at the sampling site

Characterize the integrated global properties to allow comparison with ground-based telescopic data of entire asteroid population

Measure the Yarkovsky effect

Mission Overview:

Launch in

September 2016

Encounter asteroid (101955) 1999 RQ36 in October 2019

Study RQ36 for up to 505 days, globally mapping the surface

Obtain at least 60 g of pristine regolith/surface material

Return sample to Earth in September 2023 in a Stardust-heritage capsule

Deliver samples to JSC curation facility for world-wide distribution

30

RQ36 - Apollo

r ~ 280 m

P ~ 436 daysSlide31

Discovery and New Frontiers Missions Timeline - Current Missions

8-year Phase E

Dawn

ASPERA-3

6-year Phase E

GRAIL

2009

2010

2011

2012

2013

2014

2015

2008

2007

2006

2005

2004

2003

2000

2002

2001

Strofio

Extended Mission

New Horizons

10-year Phase E

Juno

10-year Phase E

2016

2017

2018

2019

2020

2021

2009

2010

2011

2012

2013

2014

2015

2008

2007

2006

2005

2004

2003

2000

2002

2001

2016

2017

2018

2019

2020

2021

EPOXI

MESSENGER

8-year Phase E

12 month Phase E (+6 month extension)

Discovery Missions

New Frontiers Missions

Now

Phase E

Phases Pre-A,A,B,C,D

Calendar Year

Extended Mission

InSight

Extended Mission

OSIRIS-REx

2022

2022

7-year Phase E

2022

2023

HibernationSlide32

32

Mars Exploration Program 2000-2010

Follow the Water…

”Slide33

Mars Budget Analysis FY’00 through FY’

17

2000

2001

2002

2003

2004

2005

2006

2007

2008

2009

2010

2011

2012

2013

2014

2015

2016

2017

Mars Op Budget FY'00-FY'11

271

451

454

497

553

532

593

607

695

362

438

547

587

0

0

0

0

0

Mars Pres Budget FY'12-FY'17

0

0

0

0

0

0

0

0

0

0

0

0

0

361

228

189

267

503

$M

MSL Delay

MSL LandingSlide34

NASA’

s Future Mars Missions

34

MRO

Mars Express

Collaboration

Odyssey

2013

Operational

Phoenix

(completed)

2001-2012

2016

2018

2020

Curiosity

Mars Science Laboratory

MAVEN Aeronomy Orbiter

2022

ESA Trace Gas Orbiter

(Electra)

ESA ExoMars

Rover (MOMA)

2020

Science Rover

34

InSight

Future Planning

Opportunity

Spirit

(completed)

Seeking Signs of Life…

”Slide35
Slide36

Developing MissionsSlide37

Upcoming Launches

MAVEN and LADEE in final phases of development for 2013 launch datesSlide38

The JUpiter ICy moons Orbiter Mission

On May 2, 2012, the ESA formally selected JUICE as the first Large-class mission in ESA

s Cosmic Vision Program

The JUICE mission will investigate the emergence of habitable worlds around gas giants, characterizing Ganymede, Europa, and Callisto as planetary objects and potential habitats

JUICE will first orbit Jupiter for ~2.5 years, providing 13 flybys of Callisto and 2 of Europa, and then will orbit Ganymede for 9 months

Launch is scheduled for 2022 with Jupiter arrival in 2030 and Ganymede orbit insertion in 2032

NASA will contribute ~$100M in instruments and other support

38Slide39

Planetary TechnologiesSlide40

ASRG and Pu-238 Production

Advanced Stirling Radioistope Generator (ASRG)After Discovery 12 selection, working to identify next ASRG mission

Expectation is that Discovery 13 will provide similar opportunities to test mission enabling technologies (ie: ASRG, NEXT…)

Two ASRG flight units (F1 and F2) will be completed in 2016

The completed flight units will go into bonded storage, unfueled, pending a mission decision for flight use

Plutonium-238

Technology demonstration activities include:

A qualified Neptunium-237 target for irradiation

in the High Flux Isotope Reactor

(First Np-237 targets irradiated)

A qualified process for post-irradiation target processing

A qualified Pu-238 product

A project plan for scale-up to full-scale production at 1.5-2.0 kg/year

Project baseline and confirmation by December 2013Slide41

Planetary Supporting Researchand Analysis ProgramSlide42

Planetary Science Research

PGG, Cosmochem, PAST, PATM, PME, PIDDP, Origins, PP, LPI, ASTEP, ASTID, NAI, Exobiology

Near Earth Objects Observation (NEOO)

Planetary Data Systems (PDS)

Astromaterial Curation

Mars Research & Analysis

Mars Data Analysis Program (MDAP)

Mars Fundamental Research Program (MFRP)

Discovery Research

SRLI DAP/LARS (Lab Analysis of Returned Samples)

PMDAP (Planetary Missions DAP)

MESSENGER/Dawn PSP

GRAIL PSP

Outer Planets Research

OPRP, Cassini DAP/PSP

Lunar Science Research

NLSI, LASER, MMAMA, PGG/Cosmo Lunar, LRO PSP

Supporting Research & Analysis (R&A) Program Elements

Call for Proposal to these PSD Program Elements comes out in ROSESSlide43

Questions?

http://solarsystem.nasa.gov/yss

43