alaudun16.blogspot.com

Exploration

Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

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Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

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1 exploration

2 translate

3 the elysium region

4 zephyrus fossae

5 ituxi vallis

6 patapsco vallis

7 the cerberus fossae

8 zunil crater

9 orcas patera

10 rahway valles

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exploration,translate,the elysium region,zephyrus fossae,ituxi vallis,patapsco vallis,the cerberus fossae,zunil crater,orcas patera,rahway valles,posted by,anthony laudun,no comments,email this,blogthis,share to twitter,share to facebook,mars survey

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Exploration | alaudun16.blogspot.com Reviews

https://alaudun16.blogspot.com

Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

INTERNAL PAGES

alaudun16.blogspot.com

1

Exploration: November 2013

http://www.alaudun16.blogspot.com/2013_11_01_archive.html

Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

2

Exploration: Small Pale Red Planet Issue 2 Phase 8

http://www.alaudun16.blogspot.com/2013/11/small-pale-red-planet-issue-2-phase-8.html

Thursday, November 7, 2013. Small Pale Red Planet Issue 2 Phase 8. This Region contains the eastern part of the Isidis basin, a location where magnesium carbonate was found by MRO. This mineral indicates that water was present and that it was not acidic. Life may have formed in this area. There are Dark slope streaks, troughs (fossae), and river valleys (Vallis) in this Region. The Region is named for Amenthes the underworld of Ancient Egypt. Topographical Map of the Amenthes Region. A part of the Libya ...

3

Exploration: Small Pale Red Planet Issue 2 Phase 8

http://www.alaudun16.blogspot.com/2013/11/small-pale-red-planet-issue-2-phase-8_7.html

Thursday, November 7, 2013. Small Pale Red Planet Issue 2 Phase 8. This Region contains the eastern part of the Isidis basin, a location where magnesium carbonate was found by MRO. This mineral indicates that water was present and that it was not acidic. Life may have formed in this area. There are Dark slope streaks, troughs (fossae), and river valleys (Vallis) in this Region. The Region is named for Amenthes the underworld of Ancient Egypt. Topographical Map of the Amenthes Region. A part of the Libya ...

4

Exploration: September 2013

http://www.alaudun16.blogspot.com/2013_09_01_archive.html

Thursday, September 26, 2013. Small Pale Red Planet Issue 2 Phase 3.1. The Region covers the area from 90° to 135° East longitude and 0° to 30° north latitude on Mars and contains most of the Tharsis Rise. The plateau is about as high as Earth's Mount Everest and about as big in area as all of Europe. Tharsis contains a group of large volcanoes. Olympus Mons is the tallest. Topographical Map of Tharsis Region. Image of the Tharsis Region. Pangboche Crater in the Infrared at the top of Mount Olympus.

5

Exploration: Small Pale Red Planet Issue 2 Phase 9

http://www.alaudun16.blogspot.com/2013/11/small-pale-red-planet-issue-2-phase-9.html

Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

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alaudun15.blogspot.com

Exploration: Small Pale Red Planet Issue 1 Phase 12

http://alaudun15.blogspot.com/2013/09/small-pale-red-planet-issue-1-phase-12.html

Wednesday, September 4, 2013. Small Pale Red Planet Issue 1 Phase 12. Topographical Map for the Casius Region. The southern and northern borders of the Casius Region are approximately 3,065 km and 1,500 km wide, respectively. The north to south distance is about 2,050 km. (slightly less than the length of Greenland. Image of Casius Region. The Nilosyrtis Mensae Channel. Ridges in surface of Nilosyrtis Mensae. The surface of Nilosyrtis Mensae is classified as fretted terrain. This terrain contains cli...

alaudun15.blogspot.com

Exploration: Small Pale Red Planet Issue 1 Phase 13

http://alaudun15.blogspot.com/2013/09/small-pale-red-planet-issue-1-phase-13.html

Tuesday, September 10, 2013. Small Pale Red Planet Issue 1 Phase 13. Topographical Map of The Cebrenia Region showing landing site of Viking 2 Lander. The southern and northern borders of the Cebrenia Region are approximately 3,065 km (1,905 mi) and 1,500 km (930 mi) wide, respectively. The north to south distance is about 2,050 km (1,270 mi). Image of The Cebrenia Region. The Surface of Utopia Planitia. Viking 2 Lander Image. Viking 2 Lander Video. The Crater Mie Floor. The Crater Mie Floor in color.

alaudun17.blogspot.com

Exploration: November 2013

http://alaudun17.blogspot.com/2013_11_01_archive.html

Saturday, November 30, 2013. Small Pale Red Planet Issue 3 Phase 1. Leaving the Elysium Region at the southeast corner and entering the northeast corner of the Memnonia Region we begin the survey of the southern half of Mars. Topographical Map of the Memnonia Region of Mars. Image of the Memnonia Region of Mars. The first area o. F importance we encounter is the Lucus Planum. It occupies the northeast corner of the Memnonia Region. Leading to the south from the Lucus Planum is the Memnonia Sulci. William...

alaudun17.blogspot.com

Exploration: February 2014

http://alaudun17.blogspot.com/2014_02_01_archive.html

Thursday, February 27, 2014. Small Pale Red Planet Issue 3 Phase 8.1. Topographical Map of the Aeolis Region. The Aeolis quadrangle covers 180° to 225° W and 0° to 30° south on Mars. It is famous as the site of two spacecraft landings: the Spirit Rover landing site ( 14.5°S 175.4°E) in Gusev crater (January 4, 2004), and the Curiosity Rover in Gale Crater ( 4.5°S 137.4°E) (August 6, 2012). Two Rovers in the Same Region. Image of the Aeolis Region. Compaction refers to sediment that is originally porous a...

alaudun17.blogspot.com

Exploration: March 2014

http://alaudun17.blogspot.com/2014_03_01_archive.html

Thursday, March 6, 2014. Small Pale Red Planet Issue 3 Phase 8.2. Topographical Map of the Aeolis Region. The Reason this Phase has been split into two Phases (chapters) is there is a large amount of information discovered by the Curiosity and the Spirit Rovers that need to be considered. Since we are finished with Curiosity this Phase will deal with the Spirit Rover which did it’s work while it was operational on the opposite (east) side of the Aeolis Region. Depression in Avernus Cavi Region. To the ea...

alaudun17.blogspot.com

Exploration: Small Pale Red Planet Issue 3 Phase 8.1

http://alaudun17.blogspot.com/2014/02/small-pale-red-planet-issue-3-phase-81.html

Thursday, February 27, 2014. Small Pale Red Planet Issue 3 Phase 8.1. Topographical Map of the Aeolis Region. The Aeolis quadrangle covers 180° to 225° W and 0° to 30° south on Mars. It is famous as the site of two spacecraft landings: the Spirit Rover landing site ( 14.5°S 175.4°E) in Gusev crater (January 4, 2004), and the Curiosity Rover in Gale Crater ( 4.5°S 137.4°E) (August 6, 2012). Two Rovers in the Same Region. Image of the Aeolis Region. Compaction refers to sediment that is originally porous a...

alaudun17.blogspot.com

Exploration: December 2013

http://alaudun17.blogspot.com/2013_12_01_archive.html

Saturday, December 21, 2013. Small Pale Red Planet Issue 3 Phase 3.1. To begin, this Phase will be written differently than any of the other Phases before it. This is due to the west-east orientation of the Valles Marineris. Therefore we will be going from east to west and come back from west to east until this Phase ends. Normally I write each Phase in a north-south and south-north orientation, but not this time for the reasons I have given above. Topographical Map of Coprates Region. Echus Chasma is a ...

alaudun17.blogspot.com

Exploration: January 2014

http://alaudun17.blogspot.com/2014_01_01_archive.html

Monday, January 27, 2014. Small Pale Red Planet Issue 3 Phase 5. The Sinus Sabaeus Region. Topographical Map of Sinus Sabaeus Region. The Sinus Sabaeus Region covers the area from 315° to 360° west longitude and 0° to 30° degrees south latitude on Mars. Most of the region contains heavily cratered highlands. The northern part includes the huge Schiaparelli Crater. Image of Sinus Sabaeus Region. Mädler crater on Mars named is in honor of the German astronomer Johann Heinrich Mädler. The Crater is 125 ...

alaudun15.blogspot.com

Exploration: Small Pale Red Planet Issue 1 Phase 11

http://alaudun15.blogspot.com/2013/08/small-pale-red-planet-issue-1-phase-11.html

Sunday, August 25, 2013. Small Pale Red Planet Issue 1 Phase 11. Topographical Map of the Ismenius Lacus Region. The southern and northern borders of the Ismenius Lacus Region are approximately 3,065 km (1,905 mi) and 1,500 km (930 mi) wide, respectively. The north to south distance is about 2,050 km (1,270 mi). The Region covers an approximate area of 4.9 million square km, or a little over 3% of Mars’ surface area. Image of the Ismenius Lacus Region. Lyot Crater with dunes and dust devil tracks. Wide v...

alaudun15.blogspot.com

Exploration: September 2013

http://alaudun15.blogspot.com/2013_09_01_archive.html

Tuesday, September 10, 2013. Small Pale Red Planet Issue 1 Phase 13. Topographical Map of The Cebrenia Region showing landing site of Viking 2 Lander. The southern and northern borders of the Cebrenia Region are approximately 3,065 km (1,905 mi) and 1,500 km (930 mi) wide, respectively. The north to south distance is about 2,050 km (1,270 mi). Image of The Cebrenia Region. The Surface of Utopia Planitia. Viking 2 Lander Image. Viking 2 Lander Video. The Crater Mie Floor. The Crater Mie Floor in color.

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alaudun.blogspot.com

Exploration

Sunday, December 26, 2010. LInes In The Desert Plains Chapter 11: An investigation of the Nazca Lines. From 1-450 A.D. the headhunting increased and so did the fertility rituals at Cahuachi. It is believed this was one of the reasons for its abandonment. Nazca Diety with Trophy Heads. Nazca Fertility Diety pottery. Maria Rieche used the profits from her book to campaign for the preservation of the Nazca Desert. She convinced the government to restrict public access to the area. Changes to the weather all...

alaudun.wordpress.com

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Sorry, but you are looking for something that isn't here. Exploration: Maya Astronaut: Pakal the Great. Maya Astronaut: Pakal the Great Chapter 10. Maya Astronaut: Pakal the Great Chapter 9. Maya Astronaut: Pakal the Great Chapter 8. Maya Astronaut: Pakal the Great Chapter 7. Maya Astronaut: Pakal the Great Chapter 6. Maya Astronaut: Pakal the Great Chapter 5. Maya Astronaut: Pakal the Great Chapter 4. Maya Astronaut: Pakal the Great Chapter 3. Exploration: Kepler and New Horizons Missions Updates. Lines...

alaudun10.blogspot.com

Exploration

Tuesday, January 8, 2013. The Mystery of Tiwanaku / Phase 17. Original Tiwanaku -Pumapunku complex. Tiwanaku at its greatest territorial extent ca. 950 A D. Aerial View Tiwanaku Main Site (excluding Pumapunku). After 1,000 AD, the empire collapsed and complete de-urbanization occurred by 1250 A.D. Localized raised field cultivation continued, but large-scale systems were not restored. Complete Map of Tiwanaku Area. Tiwanaku / Peru pacific seacoast. Links to this post. Labels: Ancient Astronaut Theory.

alaudun15.blogspot.com

Exploration

Tuesday, September 10, 2013. Small Pale Red Planet Issue 1 Phase 13. Topographical Map of The Cebrenia Region showing landing site of Viking 2 Lander. The southern and northern borders of the Cebrenia Region are approximately 3,065 km (1,905 mi) and 1,500 km (930 mi) wide, respectively. The north to south distance is about 2,050 km (1,270 mi). Image of The Cebrenia Region. The Surface of Utopia Planitia. Viking 2 Lander Image. Viking 2 Lander Video. The Crater Mie Floor. The Crater Mie Floor in color.

alaudun16.blogspot.com

Exploration

Monday, November 18, 2013. Small Pale Red Planet Issue 2 Phase 9. The Elysium Region covers the area 180° to 225° west longitude and 0° to 30° north latitude on Mars. It contains the major volcanoes named Elysium Mons and Albor Tholus and river valleys- one of which, Athabasca Valles may be one of the youngest on Mars. On the east side is the interesting elongated depression called Orcus Patera. Topographical Map of the Elysium Region. Image of the Elysium Region. Craters and Valleys in Elysium Fossae.

alaudun17.blogspot.com

Exploration

Thursday, March 6, 2014. Small Pale Red Planet Issue 3 Phase 8.2. Topographical Map of the Aeolis Region. The Reason this Phase has been split into two Phases (chapters) is there is a large amount of information discovered by the Curiosity and the Spirit Rovers that need to be considered. Since we are finished with Curiosity this Phase will deal with the Spirit Rover which did it’s work while it was operational on the opposite (east) side of the Aeolis Region. Depression in Avernus Cavi Region. To the ea...

alaudun33.blogspot.com

Exploration

This is one story from a magazine blog. It is about exploration of the past, present, and future. Subscribe to: Posts (Atom). Http:/ alaudun4.blogspot.com. View my complete profile. Anthony Laudun. Travel template. Powered by Blogger.

alaudun4.blogspot.com

Exploration

Tuesday, February 28, 2012. First Civilization Part 1 Chapter 8. A comparison: This tells you how little we know of this planet's history:. A Martian Plant and grass. As the Surveyor came to Mars it flew into the atmosphere and began its orbit. It began to analyze the gases in the atmosphere. Record pictures of the land below the land in the south and the ocean in the northern areas. There was also plant life and animal life on the planet much of it resembling prehistoric Earth. End of Part 1. First Ci...

alaudun44.blogspot.com

Exploration

Thursday, February 27, 2014. New Horizons Mission Update 2/27/14. Beginning 1/19/06 19:00:00 UTC. 2961 Days (8.11 yrs.) 07 Hours 58 Minutes. 407 Days (1.12 yrs.) 21 Hours 01 Minutes. 501 Days (1.37 yrs.) 08 Hours 50 Minutes. New Horizons Course and Position in Two Dimensions:. Labels: Exploration: New Horizons. New Horizons Mission Update. New Horizons Update and Conference. Friday, February 7, 2014. New Horizons Mission Update 2/7/14. Beginning 1/19/06 19:00:00 UTC. Science at the Frontier:. Pluto's lar...

alaudun45.blogspot.com

Exploration

Monday, February 17, 2014. Juno Mission Update 2/17/14. Juno Mission Elapsed Time:. 2 Years 196 Days 09 Hours 59 Minutes. Time Until Arrival at Jupiter:. 2 Years 140 Days 00 Hours 05 Minutes. This is one mission that is going slow right now. What I am reporting has taken place that many people may not know completely about. I didn’t until I looked into the matter. This mission’s sites are different from that of any of the other missions I have covered or am covering now. Juno Earth Fly –by. INSTRUMENT (J...