- published: 11 Sep 2013
- views: 21
-
remove the playlistCebrenia Quadrangle
- remove the playlistCebrenia Quadrangle
Cebrenia quadrangle
The Cebrenia quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The quadrangle is located in the northeastern portion of Mars’ eastern hemisphere and covers 120° to 180° east longitude (180° to 240° west longitude) and 30° to 65° north latitude. The quadrangle uses a Lambert conformal conic projection at a nominal scale of 1:5,000,000 (1:5M). The Cebrenia quadrangle is also referred to as MC-7 (Mars Chart-7). It includes part of Utopia Planitia and Arcadia Planitia. The southern and northern borders of the Cebrenia quadrangle 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) (slightly less than the length of Greenland). The quadrangle covers an approximate area of 4.9 million square km, or a little over 3% of Mars’ surface area.
Origin of name
Cebrenia is a telescopic albedo feature centered on 50° N and 150° E on Mars. The feature is named after the plains around ancient Troy. The name was approved by the International Astronomical Union (IAU) in 1958.
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Cebrenia_quadrangle
Podcasts:
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Mars Clips 16
The Cebrenia Region Surface of Utopia Planitia
published: 11 Sep 2013 -
Mars Clips 15
The Cebrenia Region Viking 2 Lander Video
published: 11 Sep 2013 -
Fossa (planetary nomenclature) | Wikipedia audio article
This is an audio version of the Wikipedia Article: https://en.wikipedia.org/wiki/Fossa_(planetary_nomenclature) 00:00:38 1 Fossae on Mars 00:02:48 2 Fossae in the Tharsis quadrangle 00:02:58 3 Fossae in the Arcadia quadrangle 00:03:08 4 Fossae in the Elysium quadrangle 00:03:17 5 Fossae in the Mare Tyrhenum quadrangle 00:03:27 6 Fossae in Memnonia quadrangle 00:03:37 7 Fossae in the Phoenicus Lacus quadrangle 00:03:47 8 Fossae in the Diacria quadrangle 00:03:56 9 Fossae in the Phaethontis quadrangle 00:04:06 10 Fossae in the Ismenius Lacus quadrangle 00:04:16 11 Fossae in the Cebrenia quadrangle 00:04:26 12 Fossae in the Lunae Palus quadrangle Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken languag...
published: 29 May 2019 -
Water Ice on Mars
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is a large plain within Utopia, the largest recognized impact basin on Mars and in the Solar System with an estimated diameter of 3300 km.It is the Martian region where the Viking 2 lander touched down and began exploring on September 3, 1976, and the Zhurong rover touched down on 14 May, 2021, as a part of the Tianwen-1 mission.It is located at the antipode of Argyre Planitia, centered at 46.7°N 117.5°E.It is also in the Casius quadrangle, Amenthes quadrangle, and the Cebrenia quadrangle of Mars. Many rocks at Utopia Planitia appear perched, as if wind removed much of the soil at their bases.A hard surface crust is formed by solutions of minerals moving up through soil and evaporating at the surface.So...
published: 29 May 2021 -
Ring Of Saturn (Live)
Recorded Live: 02/29/20 Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the sou...
published: 01 Mar 2020 -
Live From The Ancient Mars Complex At Arcadia Planitia
Recorded Live: 02/23/20 Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the sou...
published: 02 Mar 2020 -
Mars Reconnaissance Orbiter
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory. The mission is managed by the California Institute of Technology, at the JPL, in La Cañada Flintridge, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft which were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the t...
published: 20 Oct 2015 -
Mars Reconnaissance Orbiter | Wikipedia audio article
This is an audio version of the Wikipedia Article: Mars Reconnaissance Orbiter Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago. Learning by listening is a great way to: - increases imagination and understanding - improves your listening skills - improves your own spoken accent - learn while on the move - reduce eye strain Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone. You can find other Wikipedia audi...
published: 18 Nov 2018 -
mars explored 2021 arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে Subtittle: আরেবিয়া টেরা মঙ্গল গ্রহ Mars is always in the center on human attention as a prospectful habitable planet. Terraforming mars is mans biggest dream of our present time. Nasa along with jet propultion library as of now are most advanced in exploring mars. Elon musk founder of Space X also has a vision to send one million people in mars to colonize mars. till not so many oribiter are sent to mars to understand its weather, hunt for life and water , geology and so on. from the sattelite pics mars total area is survayed. The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. Each quadrangle is a region covering a specified range of latitudes...
published: 09 Jun 2021
developed with YouTube
1:59
Mars Clips 16
- Order: Reorder
- Duration: 1:59
- Uploaded Date: 11 Sep 2013
- views: 21
The Cebrenia Region
Surface of Utopia Planitia
The Cebrenia Region
Surface of Utopia Planitia
https://wn.com/Mars_Clips_16
The Cebrenia Region
Surface of Utopia Planitia
0:48
Mars Clips 15
- Order: Reorder
- Duration: 0:48
- Uploaded Date: 11 Sep 2013
- views: 38
The Cebrenia Region
Viking 2 Lander Video
The Cebrenia Region
Viking 2 Lander Video
https://wn.com/Mars_Clips_15
The Cebrenia Region
Viking 2 Lander Video
- published: 11 Sep 2013
- views: 38
4:40
Fossa (planetary nomenclature) | Wikipedia audio article
- Order: Reorder
- Duration: 4:40
- Uploaded Date: 29 May 2019
- views: 5
This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fossa_(planetary_nomenclature)
00:00:38 1 Fossae on Mars
00:02:48 2 Fossa...
This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fossa_(planetary_nomenclature)
00:00:38 1 Fossae on Mars
00:02:48 2 Fossae in the Tharsis quadrangle
00:02:58 3 Fossae in the Arcadia quadrangle
00:03:08 4 Fossae in the Elysium quadrangle
00:03:17 5 Fossae in the Mare Tyrhenum quadrangle
00:03:27 6 Fossae in Memnonia quadrangle
00:03:37 7 Fossae in the Phoenicus Lacus quadrangle
00:03:47 8 Fossae in the Diacria quadrangle
00:03:56 9 Fossae in the Phaethontis quadrangle
00:04:06 10 Fossae in the Ismenius Lacus quadrangle
00:04:16 11 Fossae in the Cebrenia quadrangle
00:04:26 12 Fossae in the Lunae Palus quadrangle
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
Listen on Google Assistant through Extra Audio:
https://assistant.google.com/services/invoke/uid/0000001a130b3f91
Other Wikipedia audio articles at:
https://www.youtube.com/results?search_query=wikipedia+tts
Upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
Speaking Rate: 0.9816352211462827
Voice name: en-AU-Wavenet-D
"I cannot teach anybody anything, I can only make them think."
- Socrates
SUMMARY
=======
In planetary nomenclature, a fossa (pl. fossae) is a long, narrow depression (trough) on the surface of an extraterrestrial body, such as a planet or moon. The term, which means "ditch" or "trench" in Latin, is not a geological term as such but a descriptor term used by the United States Geological Survey (USGS) and the International Astronomical Union (IAU) for topographic features whose geology or geomorphology is uncertain due to lack of data or knowledge of the exact processes that formed them. Fossae are believed to be the result of a number of geological processes, such as faulting or subsidence. Many fossae on Mars are probably graben.
https://wn.com/Fossa_(Planetary_Nomenclature)_|_Wikipedia_Audio_Article
This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fossa_(planetary_nomenclature)
00:00:38 1 Fossae on Mars
00:02:48 2 Fossae in the Tharsis quadrangle
00:02:58 3 Fossae in the Arcadia quadrangle
00:03:08 4 Fossae in the Elysium quadrangle
00:03:17 5 Fossae in the Mare Tyrhenum quadrangle
00:03:27 6 Fossae in Memnonia quadrangle
00:03:37 7 Fossae in the Phoenicus Lacus quadrangle
00:03:47 8 Fossae in the Diacria quadrangle
00:03:56 9 Fossae in the Phaethontis quadrangle
00:04:06 10 Fossae in the Ismenius Lacus quadrangle
00:04:16 11 Fossae in the Cebrenia quadrangle
00:04:26 12 Fossae in the Lunae Palus quadrangle
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
Listen on Google Assistant through Extra Audio:
https://assistant.google.com/services/invoke/uid/0000001a130b3f91
Other Wikipedia audio articles at:
https://www.youtube.com/results?search_query=wikipedia+tts
Upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
Speaking Rate: 0.9816352211462827
Voice name: en-AU-Wavenet-D
"I cannot teach anybody anything, I can only make them think."
- Socrates
SUMMARY
=======
In planetary nomenclature, a fossa (pl. fossae) is a long, narrow depression (trough) on the surface of an extraterrestrial body, such as a planet or moon. The term, which means "ditch" or "trench" in Latin, is not a geological term as such but a descriptor term used by the United States Geological Survey (USGS) and the International Astronomical Union (IAU) for topographic features whose geology or geomorphology is uncertain due to lack of data or knowledge of the exact processes that formed them. Fossae are believed to be the result of a number of geological processes, such as faulting or subsidence. Many fossae on Mars are probably graben.
- published: 29 May 2019
- views: 5
2:51
Water Ice on Mars
- Order: Reorder
- Duration: 2:51
- Uploaded Date: 29 May 2021
- views: 18
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is a large plain within Utopia, the largest recognized impact basin on Ma...
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is a large plain within Utopia, the largest recognized impact basin on Mars and in the Solar System with an estimated diameter of 3300 km.It is the Martian region where the Viking 2 lander touched down and began exploring on September 3, 1976, and the Zhurong rover touched down on 14 May, 2021, as a part of the Tianwen-1 mission.It is located at the antipode of Argyre Planitia, centered at 46.7°N 117.5°E.It is also in the Casius quadrangle, Amenthes quadrangle, and the Cebrenia quadrangle of Mars.
Many rocks at Utopia Planitia appear perched, as if wind removed much of the soil at their bases.A hard surface crust is formed by solutions of minerals moving up through soil and evaporating at the surface.Some areas of the surface exhibit scalloped topography, a surface that seems to have been carved out by an ice cream scoop. This surface is thought to have formed by the degradation of an ice-rich permafrost.Many features that look like pingos on the Earth are found in Utopia Planitia (~35–50° N; ~80–115° E).[10]
On November 22, 2016, NASA reported finding a large amount of underground ice in the Utopia Planitia region. The volume of water detected has been estimated to be equivalent to the volume of water in Lake Superior.
Utopia Planitia on Mars is covered with rocks and boulders with thin layer of Water Ice by Viking 2 Lander spacecraft from NASA. High-resolution color photo of the surface of Mars was taken by Viking Lander 2 at its Utopia Planitia landing site on May 18, 1979, and relayed to Earth by Orbiter 1 on June 7. It shows a thin coating of water ice on the rocks and soil. The time the frost appeared corresponds almost exactly with the buildup of frost one Martian year (23 Earth months) ago. Then it remained on the surface for about 100 days. Scientists believe dust particles in the atmosphere pick up bits of solid water. That combination is not heavy enough to settle to the ground. But carbon dioxide, which makes up 95 percent of the Martian atmosphere, freezes and adheres to the particles and they become heavy enough to sink. Warmed by the Sun, the surface evaporates the carbon dioxide and returns it to the atmosphere, leaving behind the water and dust. The ice seen in this picture, like that which formed one Martian year ago, is extremely thin, perhaps no more than one-thousandth of an inch thick. China’s Zhurong Mars rover successfully landed in this area on May 14, and sent the first images of` its landing site in Utopia Planitia.
Credit: nasa.gov, NASA/JPL-Caltech, NASA/JPL-Caltech/ASU
https://wn.com/Water_Ice_On_Mars
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is a large plain within Utopia, the largest recognized impact basin on Mars and in the Solar System with an estimated diameter of 3300 km.It is the Martian region where the Viking 2 lander touched down and began exploring on September 3, 1976, and the Zhurong rover touched down on 14 May, 2021, as a part of the Tianwen-1 mission.It is located at the antipode of Argyre Planitia, centered at 46.7°N 117.5°E.It is also in the Casius quadrangle, Amenthes quadrangle, and the Cebrenia quadrangle of Mars.
Many rocks at Utopia Planitia appear perched, as if wind removed much of the soil at their bases.A hard surface crust is formed by solutions of minerals moving up through soil and evaporating at the surface.Some areas of the surface exhibit scalloped topography, a surface that seems to have been carved out by an ice cream scoop. This surface is thought to have formed by the degradation of an ice-rich permafrost.Many features that look like pingos on the Earth are found in Utopia Planitia (~35–50° N; ~80–115° E).[10]
On November 22, 2016, NASA reported finding a large amount of underground ice in the Utopia Planitia region. The volume of water detected has been estimated to be equivalent to the volume of water in Lake Superior.
Utopia Planitia on Mars is covered with rocks and boulders with thin layer of Water Ice by Viking 2 Lander spacecraft from NASA. High-resolution color photo of the surface of Mars was taken by Viking Lander 2 at its Utopia Planitia landing site on May 18, 1979, and relayed to Earth by Orbiter 1 on June 7. It shows a thin coating of water ice on the rocks and soil. The time the frost appeared corresponds almost exactly with the buildup of frost one Martian year (23 Earth months) ago. Then it remained on the surface for about 100 days. Scientists believe dust particles in the atmosphere pick up bits of solid water. That combination is not heavy enough to settle to the ground. But carbon dioxide, which makes up 95 percent of the Martian atmosphere, freezes and adheres to the particles and they become heavy enough to sink. Warmed by the Sun, the surface evaporates the carbon dioxide and returns it to the atmosphere, leaving behind the water and dust. The ice seen in this picture, like that which formed one Martian year ago, is extremely thin, perhaps no more than one-thousandth of an inch thick. China’s Zhurong Mars rover successfully landed in this area on May 14, and sent the first images of` its landing site in Utopia Planitia.
Credit: nasa.gov, NASA/JPL-Caltech, NASA/JPL-Caltech/ASU
- published: 29 May 2021
- views: 18
5:22
Ring Of Saturn (Live)
- Order: Reorder
- Duration: 5:22
- Uploaded Date: 01 Mar 2020
- views: 23
Recorded Live: 02/29/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in ...
Recorded Live: 02/29/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#RingsOfSaturn
#ArcadiaPlanitia
https://wn.com/Ring_Of_Saturn_(Live)
Recorded Live: 02/29/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#RingsOfSaturn
#ArcadiaPlanitia
- published: 01 Mar 2020
- views: 23
44:11
Live From The Ancient Mars Complex At Arcadia Planitia
- Order: Reorder
- Duration: 44:11
- Uploaded Date: 02 Mar 2020
- views: 46
Recorded Live: 02/23/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in ...
Recorded Live: 02/23/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#FreeRatikals
#ArcadiaPlanitia
https://wn.com/Live_From_The_Ancient_Mars_Complex_At_Arcadia_Planitia
Recorded Live: 02/23/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#FreeRatikals
#ArcadiaPlanitia
- published: 02 Mar 2020
- views: 46
35:41
Mars Reconnaissance Orbiter
- Order: Reorder
- Duration: 35:41
- Uploaded Date: 20 Oct 2015
- views: 252
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft wa...
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory. The mission is managed by the California Institute of Technology, at the JPL, in La Cañada Flintridge, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft which were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers; at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of July 2015.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
https://wn.com/Mars_Reconnaissance_Orbiter
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory. The mission is managed by the California Institute of Technology, at the JPL, in La Cañada Flintridge, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft which were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers; at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of July 2015.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
- published: 20 Oct 2015
- views: 252
37:27
Mars Reconnaissance Orbiter | Wikipedia audio article
- Order: Reorder
- Duration: 37:27
- Uploaded Date: 18 Nov 2018
- views: 57
This is an audio version of the Wikipedia Article:
Mars Reconnaissance Orbiter
Listening is a more natural way of learning, when compared to reading. Writte...
This is an audio version of the Wikipedia Article:
Mars Reconnaissance Orbiter
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
You can find other Wikipedia audio articles too at:
https://www.youtube.com/channel/UCuKfABj2eGyjH3ntPxp4YeQ
You can upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
"The only true wisdom is in knowing you know nothing."
- Socrates
SUMMARY
=======
Mars Reconnaissance Orbiter (MRO) is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory (JPL). The mission is managed by the California Institute of Technology, at the JPL, in Pasadena, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft that were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers (Spirit and Opportunity); at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of April 2018.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions. It has enough propellant to keep functioning into the 2030s.
https://wn.com/Mars_Reconnaissance_Orbiter_|_Wikipedia_Audio_Article
This is an audio version of the Wikipedia Article:
Mars Reconnaissance Orbiter
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
You can find other Wikipedia audio articles too at:
https://www.youtube.com/channel/UCuKfABj2eGyjH3ntPxp4YeQ
You can upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
"The only true wisdom is in knowing you know nothing."
- Socrates
SUMMARY
=======
Mars Reconnaissance Orbiter (MRO) is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory (JPL). The mission is managed by the California Institute of Technology, at the JPL, in Pasadena, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft that were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers (Spirit and Opportunity); at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of April 2018.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions. It has enough propellant to keep functioning into the 2030s.
- published: 18 Nov 2018
- views: 57
5:49
mars explored 2021 arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
- Order: Reorder
- Duration: 5:49
- Uploaded Date: 09 Jun 2021
- views: 117
Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Subtittle: আরেবিয়া টেরা মঙ্গল গ্রহ
Mars is always in the center on human a...
Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Subtittle: আরেবিয়া টেরা মঙ্গল গ্রহ
Mars is always in the center on human attention as a prospectful habitable planet. Terraforming mars is mans biggest dream of our present time. Nasa along with jet propultion library as of now are most advanced in exploring mars. Elon musk founder of Space X also has a vision to send one million people in mars to colonize mars. till not so many oribiter are sent to mars to understand its weather, hunt for life and water , geology and so on. from the sattelite pics mars total area is survayed. The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. Each quadrangle is a region covering a specified range of latitudes and longitudes on the Martian surface. The quadrangles are named after classical albedo features.
1. Mare boreum,
2. Diacria,
3. Arcadia,
4. Mare acidalium,
5. Ismenius lacus,
6. Casius,
7. Cebrenia,
8. Amazonis,
9. Tharsis,
10. Lunae Palus,
11. Oxia Palus,
12. Arabia
13. Syrtis Major,
14. Amenthes,
15. Elysium,
16. Memnonia,
17. Phoenicis Lacus,
18. Coprates,
19. Margaritifer Sinus,
20. Sinus Sabaeus,
21. Lapygia,
22. Mare Tyrrhenum,
23. Aeolis,
24. Phaethontis,
25. Thaaumasia,
26. Argyre,
27. Noachis,
28. Hellas,
29. Eridania,
30. Mare Australe
Arabia Terra is a large upland region in the north of Mars that lies mostly in the Arabia quadrangle, but a small part is in the Mare Acidalium quadrangle. It is densely cratered and heavily eroded. This battered topography indicates great age, and Arabia Terra is presumed to be one of the oldest terrains on the planet. It covers as much as 4,500 km (2,800 mi) at its longest extent, centered roughly at 21°N 6°E[1]Coordinates: 21°N 6°E[1] with its eastern and southern regions rising 4 km (13,000 ft) above the north-west. Alongside its many craters, canyons wind through the Arabia Terra, many emptying into the large northern lowlands of the planet, which borders Arabia Terra to the north.
Arabia contains many interesting features. There are some good examples of pedestal craters in the area. A pedestal crater has its ejecta above the surrounding terrain, often forming a steep cliff. The ejecta forms a resistant layer that protects the underlying material from erosion.Mounds and buttes on the floor of some craters display many layers. The layers may have formed by volcanic processes, by wind, or by underwater deposition.Dark slope streaks have been observed in Tikhonravov Basin, a large eroded crater. The streaks appear on steep slopes and change over time. At first they are dark, then turn a lighter color, probably by the deposition of fine, light colored dust from the atmosphere. These streaks are thought to form by dust moving downslope in a way similar to snow avalanches on Earth.
Arabia Terra was named in 1879 after a corresponding albedo feature on a map by Giovanni Schiaparelli, who named it in turn after the Arabian peninsula.
Topics Covered Here:
1. History of Mars,
2. Geography of Mars,
3. Quadrangles of Mars,
4. Naming of Arabia Terra,
5. Location of Arabia Terra,
6. Layered rock of Arabia Terra.
Tags: mars explored, arabia terra in bangla 2021, বৈচিত্রময় আরেবিয়া টেরা মঙ্গল গ্রহ, আরেবিয়া টেরা বাংলাতে ২০২১, polar ice cap, geography of mars, arcadia, mare boreum, mare acidalium, ismenius lacus, casius, cebrenia, amazonis, tharsis, lunae palus, oxia palus, syrtis major, amenthes, elysium, memnonia, phoenicis lacus, coprates, margaritifer sinus, sinus sabaeus, lapygia, mare tyrrhenum, aeolis, phaethontis, thaaumasia, argyre, noachis, hellas, Eridania, mare australe, image from mars, stepping it up in arabia terra, layers in craters in arabia terra, the landscape in arabia terra, arabia terra location, arabia terra in which planet
https://wn.com/Mars_Explored_2021_Arabia_Terra_বৈচিত্রময়_মঙ্গল_গ্রহ_আরেবিয়া_টেরা_বাংলাতে
Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Subtittle: আরেবিয়া টেরা মঙ্গল গ্রহ
Mars is always in the center on human attention as a prospectful habitable planet. Terraforming mars is mans biggest dream of our present time. Nasa along with jet propultion library as of now are most advanced in exploring mars. Elon musk founder of Space X also has a vision to send one million people in mars to colonize mars. till not so many oribiter are sent to mars to understand its weather, hunt for life and water , geology and so on. from the sattelite pics mars total area is survayed. The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. Each quadrangle is a region covering a specified range of latitudes and longitudes on the Martian surface. The quadrangles are named after classical albedo features.
1. Mare boreum,
2. Diacria,
3. Arcadia,
4. Mare acidalium,
5. Ismenius lacus,
6. Casius,
7. Cebrenia,
8. Amazonis,
9. Tharsis,
10. Lunae Palus,
11. Oxia Palus,
12. Arabia
13. Syrtis Major,
14. Amenthes,
15. Elysium,
16. Memnonia,
17. Phoenicis Lacus,
18. Coprates,
19. Margaritifer Sinus,
20. Sinus Sabaeus,
21. Lapygia,
22. Mare Tyrrhenum,
23. Aeolis,
24. Phaethontis,
25. Thaaumasia,
26. Argyre,
27. Noachis,
28. Hellas,
29. Eridania,
30. Mare Australe
Arabia Terra is a large upland region in the north of Mars that lies mostly in the Arabia quadrangle, but a small part is in the Mare Acidalium quadrangle. It is densely cratered and heavily eroded. This battered topography indicates great age, and Arabia Terra is presumed to be one of the oldest terrains on the planet. It covers as much as 4,500 km (2,800 mi) at its longest extent, centered roughly at 21°N 6°E[1]Coordinates: 21°N 6°E[1] with its eastern and southern regions rising 4 km (13,000 ft) above the north-west. Alongside its many craters, canyons wind through the Arabia Terra, many emptying into the large northern lowlands of the planet, which borders Arabia Terra to the north.
Arabia contains many interesting features. There are some good examples of pedestal craters in the area. A pedestal crater has its ejecta above the surrounding terrain, often forming a steep cliff. The ejecta forms a resistant layer that protects the underlying material from erosion.Mounds and buttes on the floor of some craters display many layers. The layers may have formed by volcanic processes, by wind, or by underwater deposition.Dark slope streaks have been observed in Tikhonravov Basin, a large eroded crater. The streaks appear on steep slopes and change over time. At first they are dark, then turn a lighter color, probably by the deposition of fine, light colored dust from the atmosphere. These streaks are thought to form by dust moving downslope in a way similar to snow avalanches on Earth.
Arabia Terra was named in 1879 after a corresponding albedo feature on a map by Giovanni Schiaparelli, who named it in turn after the Arabian peninsula.
Topics Covered Here:
1. History of Mars,
2. Geography of Mars,
3. Quadrangles of Mars,
4. Naming of Arabia Terra,
5. Location of Arabia Terra,
6. Layered rock of Arabia Terra.
Tags: mars explored, arabia terra in bangla 2021, বৈচিত্রময় আরেবিয়া টেরা মঙ্গল গ্রহ, আরেবিয়া টেরা বাংলাতে ২০২১, polar ice cap, geography of mars, arcadia, mare boreum, mare acidalium, ismenius lacus, casius, cebrenia, amazonis, tharsis, lunae palus, oxia palus, syrtis major, amenthes, elysium, memnonia, phoenicis lacus, coprates, margaritifer sinus, sinus sabaeus, lapygia, mare tyrrhenum, aeolis, phaethontis, thaaumasia, argyre, noachis, hellas, Eridania, mare australe, image from mars, stepping it up in arabia terra, layers in craters in arabia terra, the landscape in arabia terra, arabia terra location, arabia terra in which planet
- published: 09 Jun 2021
- views: 117
1:59
Mars Clips 16
The Cebrenia Region
Surface of Utopia Planitia
published: 11 Sep 2013
Mars Clips 16
Mars Clips 16
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- published: 11 Sep 2013
- views: 21
The Cebrenia Region
Surface of Utopia Planitia
0:48
Mars Clips 15
The Cebrenia Region
Viking 2 Lander Video
published: 11 Sep 2013
Mars Clips 15
Mars Clips 15
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- published: 11 Sep 2013
- views: 38
The Cebrenia Region
Viking 2 Lander Video
4:40
Fossa (planetary nomenclature) | Wikipedia audio article
This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fossa_(p...
published: 29 May 2019
Fossa (planetary nomenclature) | Wikipedia audio article
Fossa (planetary nomenclature) | Wikipedia audio article
- Report rights infringement
- published: 29 May 2019
- views: 5
This is an audio version of the Wikipedia Article:
https://en.wikipedia.org/wiki/Fossa_(planetary_nomenclature)
00:00:38 1 Fossae on Mars
00:02:48 2 Fossae in the Tharsis quadrangle
00:02:58 3 Fossae in the Arcadia quadrangle
00:03:08 4 Fossae in the Elysium quadrangle
00:03:17 5 Fossae in the Mare Tyrhenum quadrangle
00:03:27 6 Fossae in Memnonia quadrangle
00:03:37 7 Fossae in the Phoenicus Lacus quadrangle
00:03:47 8 Fossae in the Diacria quadrangle
00:03:56 9 Fossae in the Phaethontis quadrangle
00:04:06 10 Fossae in the Ismenius Lacus quadrangle
00:04:16 11 Fossae in the Cebrenia quadrangle
00:04:26 12 Fossae in the Lunae Palus quadrangle
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
Listen on Google Assistant through Extra Audio:
https://assistant.google.com/services/invoke/uid/0000001a130b3f91
Other Wikipedia audio articles at:
https://www.youtube.com/results?search_query=wikipedia+tts
Upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
Speaking Rate: 0.9816352211462827
Voice name: en-AU-Wavenet-D
"I cannot teach anybody anything, I can only make them think."
- Socrates
SUMMARY
=======
In planetary nomenclature, a fossa (pl. fossae) is a long, narrow depression (trough) on the surface of an extraterrestrial body, such as a planet or moon. The term, which means "ditch" or "trench" in Latin, is not a geological term as such but a descriptor term used by the United States Geological Survey (USGS) and the International Astronomical Union (IAU) for topographic features whose geology or geomorphology is uncertain due to lack of data or knowledge of the exact processes that formed them. Fossae are believed to be the result of a number of geological processes, such as faulting or subsidence. Many fossae on Mars are probably graben.
2:51
Water Ice on Mars
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is ...
published: 29 May 2021
Water Ice on Mars
Water Ice on Mars
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- published: 29 May 2021
- views: 18
Utopia Planitia (Greek and Latin: "Nowhere Land Plain"—loosely, the plain of paradise) is a large plain within Utopia, the largest recognized impact basin on Mars and in the Solar System with an estimated diameter of 3300 km.It is the Martian region where the Viking 2 lander touched down and began exploring on September 3, 1976, and the Zhurong rover touched down on 14 May, 2021, as a part of the Tianwen-1 mission.It is located at the antipode of Argyre Planitia, centered at 46.7°N 117.5°E.It is also in the Casius quadrangle, Amenthes quadrangle, and the Cebrenia quadrangle of Mars.
Many rocks at Utopia Planitia appear perched, as if wind removed much of the soil at their bases.A hard surface crust is formed by solutions of minerals moving up through soil and evaporating at the surface.Some areas of the surface exhibit scalloped topography, a surface that seems to have been carved out by an ice cream scoop. This surface is thought to have formed by the degradation of an ice-rich permafrost.Many features that look like pingos on the Earth are found in Utopia Planitia (~35–50° N; ~80–115° E).[10]
On November 22, 2016, NASA reported finding a large amount of underground ice in the Utopia Planitia region. The volume of water detected has been estimated to be equivalent to the volume of water in Lake Superior.
Utopia Planitia on Mars is covered with rocks and boulders with thin layer of Water Ice by Viking 2 Lander spacecraft from NASA. High-resolution color photo of the surface of Mars was taken by Viking Lander 2 at its Utopia Planitia landing site on May 18, 1979, and relayed to Earth by Orbiter 1 on June 7. It shows a thin coating of water ice on the rocks and soil. The time the frost appeared corresponds almost exactly with the buildup of frost one Martian year (23 Earth months) ago. Then it remained on the surface for about 100 days. Scientists believe dust particles in the atmosphere pick up bits of solid water. That combination is not heavy enough to settle to the ground. But carbon dioxide, which makes up 95 percent of the Martian atmosphere, freezes and adheres to the particles and they become heavy enough to sink. Warmed by the Sun, the surface evaporates the carbon dioxide and returns it to the atmosphere, leaving behind the water and dust. The ice seen in this picture, like that which formed one Martian year ago, is extremely thin, perhaps no more than one-thousandth of an inch thick. China’s Zhurong Mars rover successfully landed in this area on May 14, and sent the first images of` its landing site in Utopia Planitia.
Credit: nasa.gov, NASA/JPL-Caltech, NASA/JPL-Caltech/ASU
5:22
Ring Of Saturn (Live)
Recorded Live: 02/29/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazo...
published: 01 Mar 2020
Ring Of Saturn (Live)
Ring Of Saturn (Live)
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- published: 01 Mar 2020
- views: 23
Recorded Live: 02/29/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#RingsOfSaturn
#ArcadiaPlanitia
44:11
Live From The Ancient Mars Complex At Arcadia Planitia
Recorded Live: 02/23/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazo...
published: 02 Mar 2020
Live From The Ancient Mars Complex At Arcadia Planitia
Live From The Ancient Mars Complex At Arcadia Planitia
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- published: 02 Mar 2020
- views: 46
Recorded Live: 02/23/20
Arcadia Planitia is a smooth plain with fresh lava flows and Amazonian volcanic flows on Mars. It was named by Giovanni Schiaparelli in 1882 after the Arcadia region of ancient Greece. It dates from the Amazonian period's Arcadia formation's lava flows and small cinder cones. It includes a more recently developed large region of aeolian materials derived from periglacial processes. It is located northwest of the Tharsis region in the northern lowlands, spanning roughly the region 40-60° North and 150-180° West [citation needed] straddling partly in the Cebrenia quadrangle (MC-07), and partly in the Diacria one (MC-02), and centered at 47.2°N 184.3°E. Arcadia marks a transition from the thinly cratered terrain to its north and the very old cratered terrain to the south. On its east it runs into the Alba Mons volcanoes. Its elevation relative to the geodetic datum varies between 0 and -3 km.
In a lot of the low areas of Arcadia, one finds grooves and sub-parallel ridges. These indicate movement of near surface materials and are similar to features on earth where near surface materials flow together very slowly as helped by the freezing and thawing of water located between ground layers. This supports the proposition of ground ice in the near surface of Mars in this area. This area represents an area of interest for scientists to investigate further.
Bass/Vocals: Brandon Stuck
Guitar/Vocals: Eaamon O'Shea
Drums/Vocals: Jared Inman
#FreeRatikalsSaturatedEnergyBand
#FreeRatikals
#ArcadiaPlanitia
35:41
Mars Reconnaissance Orbiter
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissanc...
published: 20 Oct 2015
Mars Reconnaissance Orbiter
Mars Reconnaissance Orbiter
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- published: 20 Oct 2015
- views: 252
Mars Reconnaissance Orbiter is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory. The mission is managed by the California Institute of Technology, at the JPL, in La Cañada Flintridge, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft which were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers; at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of July 2015.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions.
This video is targeted to blind users.
Attribution:
Article text available under CC-BY-SA
Creative Commons image source in video
37:27
Mars Reconnaissance Orbiter | Wikipedia audio article
This is an audio version of the Wikipedia Article:
Mars Reconnaissance Orbiter
Listeni...
published: 18 Nov 2018
Mars Reconnaissance Orbiter | Wikipedia audio article
Mars Reconnaissance Orbiter | Wikipedia audio article
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- published: 18 Nov 2018
- views: 57
This is an audio version of the Wikipedia Article:
Mars Reconnaissance Orbiter
Listening is a more natural way of learning, when compared to reading. Written language only began at around 3200 BC, but spoken language has existed long ago.
Learning by listening is a great way to:
- increases imagination and understanding
- improves your listening skills
- improves your own spoken accent
- learn while on the move
- reduce eye strain
Now learn the vast amount of general knowledge available on Wikipedia through audio (audio article). You could even learn subconsciously by playing the audio while you are sleeping! If you are planning to listen a lot, you could try using a bone conduction headphone, or a standard speaker instead of an earphone.
You can find other Wikipedia audio articles too at:
https://www.youtube.com/channel/UCuKfABj2eGyjH3ntPxp4YeQ
You can upload your own Wikipedia articles through:
https://github.com/nodef/wikipedia-tts
"The only true wisdom is in knowing you know nothing."
- Socrates
SUMMARY
=======
Mars Reconnaissance Orbiter (MRO) is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory (JPL). The mission is managed by the California Institute of Technology, at the JPL, in Pasadena, California, for the NASA Science Mission Directorate, Washington, D.C. It was launched August 12, 2005, and attained Martian orbit on March 10, 2006. In November 2006, after five months of aerobraking, it entered its final science orbit and began its primary science phase. As MRO entered orbit, it joined five other active spacecraft that were either in orbit or on the planet's surface: Mars Global Surveyor, Mars Express, 2001 Mars Odyssey, and the two Mars Exploration Rovers (Spirit and Opportunity); at the time, this set a record for the most operational spacecraft in the immediate vicinity of Mars. Mars Global Surveyor and the Spirit rover have since ceased to function; the remainder remain operational as of April 2018.
MRO contains a host of scientific instruments such as cameras, spectrometers, and radar, which are used to analyze the landforms, stratigraphy, minerals, and ice of Mars. It paves the way for future spacecraft by monitoring Mars' daily weather and surface conditions, studying potential landing sites, and hosting a new telecommunications system. MRO's telecommunications system will transfer more data back to Earth than all previous interplanetary missions combined, and MRO will serve as a highly capable relay satellite for future missions. It has enough propellant to keep functioning into the 2030s.
5:49
mars explored 2021 arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
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published: 09 Jun 2021
mars explored 2021 arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
mars explored 2021 arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
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- published: 09 Jun 2021
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Tittle: # mars explored 2021- arabia terra বৈচিত্রময় মঙ্গল গ্রহ আরেবিয়া টেরা বাংলাতে
Subtittle: আরেবিয়া টেরা মঙ্গল গ্রহ
Mars is always in the center on human attention as a prospectful habitable planet. Terraforming mars is mans biggest dream of our present time. Nasa along with jet propultion library as of now are most advanced in exploring mars. Elon musk founder of Space X also has a vision to send one million people in mars to colonize mars. till not so many oribiter are sent to mars to understand its weather, hunt for life and water , geology and so on. from the sattelite pics mars total area is survayed. The surface of Mars has been divided into thirty cartographic quadrangles by the United States Geological Survey. Each quadrangle is a region covering a specified range of latitudes and longitudes on the Martian surface. The quadrangles are named after classical albedo features.
1. Mare boreum,
2. Diacria,
3. Arcadia,
4. Mare acidalium,
5. Ismenius lacus,
6. Casius,
7. Cebrenia,
8. Amazonis,
9. Tharsis,
10. Lunae Palus,
11. Oxia Palus,
12. Arabia
13. Syrtis Major,
14. Amenthes,
15. Elysium,
16. Memnonia,
17. Phoenicis Lacus,
18. Coprates,
19. Margaritifer Sinus,
20. Sinus Sabaeus,
21. Lapygia,
22. Mare Tyrrhenum,
23. Aeolis,
24. Phaethontis,
25. Thaaumasia,
26. Argyre,
27. Noachis,
28. Hellas,
29. Eridania,
30. Mare Australe
Arabia Terra is a large upland region in the north of Mars that lies mostly in the Arabia quadrangle, but a small part is in the Mare Acidalium quadrangle. It is densely cratered and heavily eroded. This battered topography indicates great age, and Arabia Terra is presumed to be one of the oldest terrains on the planet. It covers as much as 4,500 km (2,800 mi) at its longest extent, centered roughly at 21°N 6°E[1]Coordinates: 21°N 6°E[1] with its eastern and southern regions rising 4 km (13,000 ft) above the north-west. Alongside its many craters, canyons wind through the Arabia Terra, many emptying into the large northern lowlands of the planet, which borders Arabia Terra to the north.
Arabia contains many interesting features. There are some good examples of pedestal craters in the area. A pedestal crater has its ejecta above the surrounding terrain, often forming a steep cliff. The ejecta forms a resistant layer that protects the underlying material from erosion.Mounds and buttes on the floor of some craters display many layers. The layers may have formed by volcanic processes, by wind, or by underwater deposition.Dark slope streaks have been observed in Tikhonravov Basin, a large eroded crater. The streaks appear on steep slopes and change over time. At first they are dark, then turn a lighter color, probably by the deposition of fine, light colored dust from the atmosphere. These streaks are thought to form by dust moving downslope in a way similar to snow avalanches on Earth.
Arabia Terra was named in 1879 after a corresponding albedo feature on a map by Giovanni Schiaparelli, who named it in turn after the Arabian peninsula.
Topics Covered Here:
1. History of Mars,
2. Geography of Mars,
3. Quadrangles of Mars,
4. Naming of Arabia Terra,
5. Location of Arabia Terra,
6. Layered rock of Arabia Terra.
Tags: mars explored, arabia terra in bangla 2021, বৈচিত্রময় আরেবিয়া টেরা মঙ্গল গ্রহ, আরেবিয়া টেরা বাংলাতে ২০২১, polar ice cap, geography of mars, arcadia, mare boreum, mare acidalium, ismenius lacus, casius, cebrenia, amazonis, tharsis, lunae palus, oxia palus, syrtis major, amenthes, elysium, memnonia, phoenicis lacus, coprates, margaritifer sinus, sinus sabaeus, lapygia, mare tyrrhenum, aeolis, phaethontis, thaaumasia, argyre, noachis, hellas, Eridania, mare australe, image from mars, stepping it up in arabia terra, layers in craters in arabia terra, the landscape in arabia terra, arabia terra location, arabia terra in which planet
Cebrenia quadrangle
The Cebrenia quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The quadrangle is located in the northeastern portion of Mars’ eastern hemisphere and covers 120° to 180° east longitude (180° to 240° west longitude) and 30° to 65° north latitude. The quadrangle uses a Lambert conformal conic projection at a nominal scale of 1:5,000,000 (1:5M). The Cebrenia quadrangle is also referred to as MC-7 (Mars Chart-7). It includes part of Utopia Planitia and Arcadia Planitia. The southern and northern borders of the Cebrenia quadrangle 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) (slightly less than the length of Greenland). The quadrangle covers an approximate area of 4.9 million square km, or a little over 3% of Mars’ surface area.
Origin of name
Cebrenia is a telescopic albedo feature centered on 50° N and 150° E on Mars. The feature is named after the plains around ancient Troy. The name was approved by the International Astronomical Union (IAU) in 1958.
This page contains text from Wikipedia, the Free Encyclopedia - https://wn.com/Cebrenia_quadrangle
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