PHOTOMAP - ELTE

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280° 300° 320° 340° 20° 40° 60° 80° 200° 220° 240° 260° 140° 160° 180° 120° 100° 40° 20° 60° 80° 80° 60° 40° 20° 20° 40° 60° 80° 80° 60° 40° 20° 20° 40° 60° 80° 80° 60° 40° 20° 20° 40° 60° 80° 80° 60° 40° 20° S S N N O l y m p u s M o n s V a s t i t a s B o r e a l i s A r c a d i a P l a n i t i a A m a z o n P l a n i t i a Lucus Pla n u m T e m p e T e r r a L u n a e P l a n u m X a n t h e T e r r a C h r y s e P l a n i t i a A c i d a l i a P l a n i t i a A r ab i a T e r r a E l y s i u m P l a n i t i a I s i d i s P l a n i t i a I s i d i s P l a n i t i a T h a r s i s M o n t e s Da e d a l i a P l a n u m T e r r a S i r e n u m I c ar i a P l a n u m S y ria P l a n u m Sin ai P l a n u m Solis Planu m V A L L E S M A R I N E R I S Thaumasia Planu m Bosporos Plan u m A o n i a T e r r a A r g y r e P l a n i t i a N o a c h i s T e r r a S a b a T e r r a S y r t i s M a j o r P l a n u m T e r r a T y r r h e n a H e s p e r i a P l a n u m P r o m e t h e i T e r r a C i m m e r i a T e r r a Planu m A u st r a l e Prometh ei P l . Parva Pla n u m P l a n u m B o r e u m S i s y p h i T e r r a He l l a s P l a n i t i a 21287 Ascraeus M ons 18229 Pavonis Mons 14057 Arsia Mons 17780 Biblis Patera Ulysses Patera Gordii D orsu m Uranius Pater a Tharsis Tholu s 4600 Uranius Tholus 4700 Ceraunius Tholus 8000 8 7 0 0 Alba Pater a 6700 A l b a F o s s a e Tantalus Fossa e N o c t i s L a b y r i n t h u s C l a r i t a s F o s s a e M e m n o n i a F o s s a e S i r e n e u m F o s s a e NEWTON C OPERNICU S · Charlier · S uess · S to n e y Gorgonum Chaos 3500 N e r e i d u m M o n t e s C h a r i t u m M o n t e s · P hillip s · Du Toit · Joly · Dana · M c M u r d o · L y e ll · S o u t h · M ain · Michel · Gilbert · B arn ar d · H olm es · Vishniac · Galle · Green Wegener · · Darwin · Lohse · Hartwig · Roddenberry · Vogel · Shatskiy · Novara · Peta · Cartago · Lorika · N o m a · Ostrov · Foros · Mena · Arkhangelsky · Helmholz · Wirtz · Maraldi · Fontana · Bozkir · Hooke Holden · · Schmidt Frigores Cavi Angusti Cavi · v o n K ár m á n · Eger · H alle y · Babakin · Lassel · Ibragim ov · Ritchey · Bunge · Hale · Bond · Jones · C h e k a l i n · K a s i m o v · Sumgin · D o u g la s s Silpher · LO W E L L U z b o i V a l l i s Nirgal Vallis S a m a r a V a lle s Eos Chasm a Capri Chasm a G anges Chasma Coprates Chasma C oprates Catena M elas Chasm a Ius Chasma H e b e s C h . K a s e i V a l l e s K a s ei V a ll e s M aja Vallis N a nedi Vallis Shalbatama Vallis · Mutch Orson Welles · Da Vinci · Perrotin · T iu V allis Ares Vallis A r e s V a l l i s Aram Chaos · Crommelin · McLaughin · Bequerel · Sklodowska Maggini · · Rutherford · Trouvelot · Radau · Marth · Gill · Pasteur Janssen · · Flammarion · Schöner · Baldet Peridier · Teisserenc de Bort · Fournier Jarry Desloges · Suzby · Kasabi · · Isil Schroeter · Verlaine · K unowski L Y O T Lomonosov Curie Cerulli A NTONIADI · Airy · Mädler Newcomb · Beer SCHIAPARELLI M e ri d ia n i P la n u m E v r o s V a l l i s · Pollack · Denning · Bouguer · Wislicenus · Le Verrier Bakhuysen · · Lambert · Flaugegues · Kaiser · Russell · Proctor · Rabe H e l l e s p o n t u s M o n t e s 8200 +MARS–2 1971† M a le a P l a n u m Patera Amphirites P r o m e t h e i R u p e s D a o - v . N i g e r V a l l i s H a r m a k h i s V . R e u ll V a l l i s R e u ll V a llis Tyrrhena Patera * * · Tikhov · Krishtofovich · Sebec G u n n is o n · · S e c c h i · H uxley · Heinlein · Byrd Jeans · · Weinbaum W ells · W a ll a c e · A rr h enius · A. Tolstoy · E r i d a nia S c o p u l u s Liais · Hutton · Burro u g h s · Eddie N e p e n thes Mensae A eolis M en sa e Gale Lasswitz Wien Knobel Albor Tholus Hecates Tholus Elysium M ons 3800 14126 4700 H r a d V a l l i s E l y s i um C h a sma M ie VIKIN G2 + 1 9 7 6 Milankovic · Korolev Stokes Tyndall Adams Lockyer Phlegra M ontes T artarus M o ntes O rc u s P a t e r a Cerberus Fossae Hibes M onte s Apollinaris Apollinaris Tholus Patera 3100 · Gusev · Molesworth · Martz · Cruls · Rossby · · Campbell · M endel · M agelhaens · Columbus P tolemaeus · · Li Fan H ipparchus · · Eudoxus · Pickering · Kuiper · Wright · N ansen · Millm an · Williams · Burton · M arca K ov alsky C o mas Sola · · Dejnev Liu Hsin · Bjerknes · Huggins T ycho Brahe · SPIRIT+ 2004 A l- Q a h i r a V a llis D r a v a V a l l e s Planum Chroniu m P O L A R L A N D E R + M ARS 1999M e d u sae F ossa e M a n g a l a V a ll e s N icholson Pettit E re b u s M . A c h eron Fossa e Mareotis Fossae Tempe Fossae Fesenkov + VIKING1 + PATHFINDER 1976 1997 M a r g a r i t i f e r T e r r a OPPORTUNITY + 2004 1974+ MARS6 C y d o nia M ensae B o re ale C h a s m a D euteronilus Mensae Protonilus Mensae N ilo sy rtis M e n s a e H u o H s i n g V a l l i s N ili F o s s a e 3 9 0 0 Nili Patera Meroe Patera 2300 L i b y a M . · Quenisset · Moreux Rudaux · · Luzin · Henry · Tikhonravov Dawes · HUYGENS CASSINI Indus Valli s Nakton g V a l l i s KEPLER HERSCHEL · Igal S a vich · · Du Matheray · Bak + BEAGLE2 2003Diacria Patera * L y c u s S u l c i O ly m p u s R u p e s Ulysses F o s s a e Gigas Sulci A g anip pe F o s s a · Poynting O udemans · Jovis Tholus * O l y m p ic a F o s s a e Tractus Catena Ceraunius Fossae AlbaCatena Acheron Catena A scuris Plan u m Perepelkin · Timoshenko · Sytinskaya · Sharanov · Chia N il o k e r a s S c o p u l u s L o b o V a l l i s Luna Mensa Bahram Vallis S acra M e n s a S a c r a F o s s a e L a b eatis Fossa EchusChasma O p h ir C h . C a n d o r C h . Tithoniae Catena Tithonium Chasm a Solis Dorsa J u v e n t a e C h . O p h i r P l a n u m A u rora e P l a n u m Aurorae Chaos Hydraotes Chaos Aureum Chaos Asrinoses Chaos Pyrrhae Chaos Margaritifer IaniChaos Chaos Simud Vallis · Marursky · Sagan · Galilaei · Timbuktu · Paks C h alco p oro s R u p e s Alpheus Colles C o r o n a e S c o p u l u s · Terby Niesten · · Schaeberle S c y l l a S c o p u l u s Charybdis Scopulu s Acidalia Colles Acidalia Mensa M a m e r s V a ll e s I s m e n i a e F o s s a e Coloe Fossae · Renaudot Nili Colles A u q a k u h - v . Nier H y b l a e u s F o s s a e E lysiu m F o s s a e S c a n d i a C o l l e s M a r t e V a l l i s Eum enides D o r s u m F o r t u n a F o s s a e Tiu Vallis M a w r t h V a ll is * * Amenthes Fossae H e p h a e s t u s F o s s a e G r a n i c u s V a ll e s Tartarus Colles R euyl de Vaucouleurs B oeddicker H adley · G raff · M üller · Ausonia M. Hadriaca Patera M o r p h e o s R u p e s C olles Ariadnes V ery · M ariner · · Bernard C obres · · C lark · D okuchaev · C h a m berlin · S te no · Smith H e a v yside · Lau · · Hus s e y · B rashear · R o ss · P o rter I caria Fossae Coracis Fossae Bosporos R u p es N e c t a r i s - F o s s a e O g y g i s R u p es L a d o n V . Fossa Ery thraea Argyre Rupes Argentea Planum · Agassiz Sisy p hi C a v i Sis y p h i M o n t e s A u s t r a l e M . P i t y u s a P a t e r a M a l e a P a t e r a P e n e u s P a t e r a Brevia Dorsum * * * * Mad Vallis Auxias Valles O e n o t r i a S c o p u l u s T h yles R u p e s U ly xis R u p e s · Richard s o n · R eyn old s · T ru m per Tempe Fossae Nilus C h a o s Mensa Tempe Nilokeras Mensae Maja V . Ganges Catena L ouros Valles Eos C h a o s Vinogradov Tisia Valles Oxia Colles B r a z o s V a l l e s Mosa Vallis P a r a n a V . H i m e r a V . L oire V a l l i s Arena C olle s Arnus Vallis Coronae M onte s Liris V alle s L o c r a s V a lle s C u s u s V a l l e s U t o p i a P l a n i t i a V a s t i t a s B o r e a l i s U t o p i a P l a n i t i a Zephiria Mensae M a a d i m V a l l i s D u ri u s - v . Atlantis- Chaos Thaumasia Fossa e Dzigai V . P a ll a c o p a s V allis Doaus Vallis D a o V a llis H e ll a s M . E u r i p u s M o n s Tader Valle s O l y m p i a U n d a e H y p e r b o r e a e U n d a e P la n u m B o re u m Escorial Abalos Und a e P r o m e t h e i R u p e s H y p e r n o t i u s S c. Australe Chasma Osuga V. Her Desher Valli s Galaxias Fluctus Baphyras- kráterlánc Rubicon Valles Ravius Valles Tanaica M. Gandzani · Semeykin MARS Solar Distance: 206–249 million km Earth Distance: 54–401 million km Equatorial Radius: 3396.2 km Obliquity to orbit: 25°19’ (±10°) Orbital Period: 668.59 Mars Day (668.59 Sol) (=687 Earth Day) Rotational Period (1 sol): 24h:37m Gravity: 0.38 g Length of Equator: 21 300 km Surface Area: 144.2 million km 2 Atmosphere: 95% CO 2 ; 2,6% N 2 Pressure: 6 mbar [min: 0,7–Olym pus, max: 12–Hellas) 0. Longitude: Airy-0 crater Height Datum 3396 km radius Distance from Earth at Light speed : 03:02–22:19 min. Solar Distance: 589.2 W/m 2 Satellites: Phobos, Deimos M 1:320 000 000 1 cm = 320 km PHOTOMAP OF MARS Showing albedo features of the surface Lambert Transversal Equivalent Azimuthal Projection Published by Eötvös Loránd University Cosmic Materials Space Research Group, Budapest, Hungary http://planetologia.elte.hu Source: Viking Orbiter Map © Henrik Hargitai 2008 ISBN HU 978-963-463-969-5 MARS FACTS CLIMATE PHOTOMAP METEO DATA EÖTVÖS L. UNIVERSITY COSMIC MATERIALS SPACE RESEARCH GROUP BUDAPEST, HUNGARY K o n k o l y T h e g e M i k l ó s 1 8 7 7 S c h i a p a r e lli 1 8 8 8 F l a m m a rio n s m a p / H u n g a ria n 1 8 7 7 VIEW OF CHRYSE PLANITIA (Viking–1) VIEW OF UTOPIA PLANITIA (Viking–2) Lowest nighttime temperature [K] Highest daytime temperatures during one Mars year [K] Ls 0 30 60 90 120 150 180 210 240 270 300 330 350 Sol 1 61 126 193 257 317 371 421 468 514 562 612 668 1 61 126 193 257 317 371 421 468 514 562 612 668 Ls 0 30 60 90 120 150 180 210 240 270 300 330 350 During one Martian year measured at 0° longitude, various latituted. Source: MGS TES Jun 2000. - Apr. 2002. Temperature 56-sol months (1=Ls 270) Line refers to the max. extent of frost cover φ 80 70 60 50 40 30 20 10 0 10 20 30 40 50 60 70 80 φ 80 70 60 50 40 30 20 10 0 10 20 30 40 50 60 70 80 K 303 293 283 273 263 258 253 243 213 203 183 173 163 153 148 143 °C 30 20 10 0 -10 -15 -20 -30 -60 -70 -90 -100 -110 -120 -125 -130 Legend 40 20 0 -20 -40 -60 -80 -100 -120 -140 1 2 3 4 5 6 7 8 9101112 60°N 56-sol months (1=Ls 270) 40 20 0 -20 -40 -60 -80 -100 -120 -140 1 2 3 4 5 6 7 8 9101112 30°N 56-sol months (1=Ls 270) 40 20 0 -20 -40 -60 -80 -100 -120 -140 1 2 3 4 5 6 7 8 9101112 56-sol months (1=Ls 270) 40 20 0 -20 -40 -60 -80 -100 -120 -140 7 8 9 101112 1 2 3456 56-sol months (1=Ls 270) 40 20 0 -20 -40 -60 -80 -100 -120 -140 K 313 293 270 253 233 213 193 173 153 133 7 8 9 101112 1 2 3456 30°S 60°S Duststorm→ dailtime max. dailtime max. dailtime max. dailtime max. nighttime min. nighttime min. nighttime min. nighttime min. nighttime min. Duststorm→ Duststorm→ Duststorm→ 90° 180° 270° Ls 0° DAILY SOLAR ENERGY AT VARIOUS LATITUDES [Wh/sol·m 2 ] 45° -45° 85° -85° 1400 1000 600 200 0 20 0 10 mb 0 mb 90° 180° 270° Ls 0° TEMPERATURE [C°] Viking–2, 47°N WIND SPEED [m/s] Viking–2, 47°N 2 2,5 SOLAR DISTANCE (million km) PRESSURE [mbar] Viking–2, 47°N -20 -40 -60 -80 -100 -120 d a il y m i n . d a il y m a x . 90° 180° 270° Ls 0° 90° 180° 270° Ls 0° 90° 180° 270° Ls 0° dust storm season Southern CO 2 frost sublimated Southern CO 2 -frost precipitated SPRING SUMMER AUTUMN WINTER Change of seasons on Mars is expressed as Ls degrees (Solar Longitude: distance of the Sun from the first point of Aries). Seasonal changes are caused not only by the tilt of axis, but also by the Solar distance, which is a major factor because of the highly elliptical orbit of Mars. This plays a major role on the actual extent of the polar (frost) caps. Southern seasons are extreme: Summer is while Mars is close to to Sun (perihelion), Winter is while far from the Sun (aphelion). Northern seasons are less different: Winter is in perihelion. The basis (x axis) of the diagrams shown here is not Ls, but a 56-sol month. The southern Summer is the season for global dust storms. The almost always cloudless sky of Mars is pale pink in colour because of the dust. During the winter, CO 2 is precipitated as frost, even at 50° lat. By summer, this sublimates, adding to global atmospheric pressure and making strong winds. South North North North North

Transcript of PHOTOMAP - ELTE

Page 1: PHOTOMAP - ELTE

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Fossae

Ogygis Rupes

Ladon V.

Fossa

Erythraea

Argyre Rupes

Argentea Planum

· Agassiz

Sisyphi Ca

vi

SisyphiMontes

AustraleM.

Pityus

a Patera Malea

Patera

Peneu

s Patera

Brevia Dorsum

**

**

Mad Vallis

AuxiasValles

Oen

o t r i aSco pu l u s

Thyles Rupes

Ulyxis Rupes

· Richardson· Reynolds

· Trumper

TempeFos

sae

Nilus Chaos

MensaTempe

NilokerasMensae

Maja V.

Ganges Catena

Louros Valles

Eos Chaos

Vinogradov

TisiaValles

OxiaColles

Brazos V

alles

Mosa Vallis

Parana V.

Him

eraV.

Loire Vallis

Arena Colles

Arnus Vallis

Coronae M

ontes

Liris Valles

Locras Valles

Cusus Valles

U t o p i a P l a n i t i a

V a s t i t a s B o r e a l i s

U t o p i aP l a

n it i

a

Zephiria Mensae

Ma’adim

Vallis

Durius-v.

Atlantis-Chaos

Thaumasia

Fossa

eDzigai V.

Pallacopa

s Vall

is

Doaus Vallis

Dao Vallis

Hellas M.

Euripu

s Mons

Tader Valles

O l y m p i a U n d a e

H y p e r b o r e a e U n d a e

PlanumBoreum

Escorial

AbalosUndae

Prom

eth

ei Rupes

Hyp

erno

tius Sc.

Australe Chasma

Osuga V.

Her Desher Vallis

Galaxias Fluctus

Baphyras-

kráterlánc

Rubicon Valles

Ravius Valles Tanaica M.

Gandzan

i ·

Semeykin

MARS

Solar Distance: 206–249 million kmEarth Distance: 54–401 million kmEquatorial Radius: 3396.2 kmObliquity to orbit: 25°19’ (±10°)Orbital Period: 668.59 Mars Day(668.59 Sol) (=687 Earth Day)Rotational Period (1 sol): 24h:37mGravity: 0.38 gLength of Equator: 21 300 kmSurface Area: 144.2 million km2Atmosphere: 95% CO2; 2,6% N2Pressure: 6 mbar [min: 0,7–Olym pus,max: 12–Hellas)0. Longitude: Airy-0 craterHeight Datum 3396 km radiusDistance from Earth at Lightspeed : 03:02–22:19 min.Solar Distance: 589.2 W/m2Satellites: Phobos, Deimos

M 1:320 000 0001 cm = 320 km

PHOTOMAP OF MARSShowing albedo features of the surface

Lambert Transversal Equivalent Azimuthal Projection

Published by Eötvös Loránd UniversityCosmic Materials Space Research Group,

Budapest, Hungaryhttp://planetologia.elte.huSource: Viking Orbiter

Map © Henrik Hargitai 2008ISBN HU 978-963-463-969-5

MARS FACTS CLIMATE

P H O T O M A P

METEO DATA

EÖTVÖS L. UNIVERSITYCOSMIC MATERIALSSPACE RESEARCH GROUPBUDAPEST, HUNGARY

Konkoly

Thege

Miklós 1877

Schiaparel

li 1888

Flamm

arion’smap

/ Hungarian 1877

VIEW OF CHRYSE PLANITIA (Viking–1) VIEW OF UTOPIA PLANITIA (Viking–2)Lowest nighttime temperature [K] Highest daytime temperatures during one Mars year [K]

Ls 0 30 60 90 120 150 180 210 240 270 300 330 350

Sol 1 61 126 193 257 317 371 421 468 514 562 612 668 1 61 126 193 257 317 371 421 468 514 562 612 668

Ls 0 30 60 90 120 150 180 210 240 270 300 330 350During one Martian year measured at 0° longitude, various

latituted. Source: MGS TES Jun 2000. - Apr. 2002.

Temperature

56-sol months (1=Ls 270)

Line refers to the max. extent of frost coverφ

807060504030201001020304050607080

φ807060504030201001020304050607080

K303293283273263258253243213203183173163153148143

°C3020100

-10-15-20-30-60-70-90-100-110-120-125-130

Legend

40200

-20-40-60-80-100-120-140

1 2 3 4 5 6 7 8 9 101112

60°N

56-sol months (1=Ls 270)

40200

-20-40-60-80-100-120-140

1 2 3 4 5 6 7 8 9 101112

30°N

56-sol months (1=Ls 270)

40200

-20-40-60-80-100-120-140

1 2 3 4 5 6 7 8 9 101112

56-sol months (1=Ls 270)

40200

-20-40-60-80-100-120-140 7 8 9 101112 1 2 3 4 5 6

56-sol months (1=Ls 270)

40200

-20-40-60-80-100-120-140

K3132932702532332131931731531337 8 9 101112 1 2 3 4 5 6

30°S 60°S

Duststorm→

dailtime max.dailtime max.

dailtime max.

dailtime m

ax.

nighttime min. nighttime min. nighttime min.nighttime min.nighttime min.

Duststorm→ Duststorm→ Duststorm→

0° 90° 180° 270° Ls 0°

DAILY SOLAR ENERGY AT VARIOUS LATITUDES [Wh/sol·m2]

45°-45°

85° -85°

1400

1000

600

200

0

20

0

10 mb

0 mb0° 90° 180° 270° Ls 0°

TEMPERATURE [C°] Viking–2, 47°N

WIND SPEED [m/s] Viking–2, 47°N

2

2,5

SOLAR DISTANCE (million km)

PRESSURE [mbar] Viking–2, 47°N

-20-40-60-80-100-120

daily min.

daily max.

0° 90° 180° 270° Ls 0°

0° 90° 180° 270° Ls 0°

0° 90° 180° 270° Ls 0°

dust storm season

Southern CO2 frostsublimatedSouthern CO2-frostprecipitated

SPRING SUMMER AUTUMN WINTER

Change of seasons on Mars is expressed as Lsdegrees (Solar Longitude: distance of the Sun from thefirst point of Aries).Seasonal changes are caused not only by the tilt of axis,but also by the Solar distance, which is a major factorbecause of the highly elliptical orbit of Mars. This playsa major role on the actual extent of the polar (frost)caps. Southern seasons are extreme: Summer is whileMars is close to to Sun (perihelion), Winter is while farfrom the Sun (aphelion). Northern seasons are lessdifferent: Winter is in perihelion. The basis (x axis) ofthe diagrams shown here is not Ls, but a 56-sol month. The southern Summer is the season for global duststorms. The almost always cloudless sky of Mars is palepink in colour because of the dust. During the winter,CO2 is precipitated as frost, even at 50° lat. By summer,this sublimates, adding to global atmospheric pressureand making strong winds.

South

North North

North North