{"id":436059,"date":"2018-05-20T16:18:03","date_gmt":"2018-05-20T16:18:03","guid":{"rendered":"https:\/\/essaypaper.org\/mars-expository-essay-samples\/"},"modified":"2018-10-24T09:04:53","modified_gmt":"2018-10-24T09:04:53","slug":"mars-expository-essay-samples","status":"publish","type":"post","link":"https:\/\/www.benedictsol.com\/blogs\/mars-expository-essay-samples\/","title":{"rendered":"Mars : Expository Essay Samples"},"content":{"rendered":"
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\"\"Mars is featured in countless science-fiction books, non-fiction books, cartoons, films, and more. However, how much do we know about the Red Planet? I would say that the average person only has a cursory knowledge of this important part of our solar system. Therefore, I will do justice to this planet by providing details about it so that the mystery of Mars can be deshrouded. I will go over its technical information, such as its general description, internal structure, surface geology, soil, hydrology, geography, atmosphere, climate, orbit, and habitability. <\/p>\n

Mars is the fourth planet from the Sun in our solar system. It is also the second-smallest planet in our solar system. By diameter, Mars is half as small as Earth, and is also less dense than Earth (Williams, David R.). Mars is named after the Roman god of war, and is often called the \u201cRed Planet\u201d (Zubrin, Robert; Wagner, Richard ). <\/p>\n

Similar to Earth, Mars has a dense metallic core with less dense material surrounding it (Nimmo, Francis; Tanaka, Ken). Its core has a radius of approximately 1,794 \u00b1 65 kilometers (1,115 \u00b1 40 mi), mostly comprising of iron and nickel, with a bit of sulfur (Rivoldini, A., et al.). By estimates, the core is about twice as rich in lighter material than Earth (Jacqu\u00e9, Dave). Though dormant, there is a silicate mantle that overlays the core, which created the tectonic plates on the planet.<\/p>\n

The surface geology of Mars is similar to Earth, with some nuances. Like Earth, Mars is a terrestrial planet, meaning that its surface is mostly composed of minerals, oxygen, metals and other substances that comprise rock. The main material the surface of Mars is made of is tholeiitic basalt (McSween, Harry Y, et al.), and most of the surface is covered in granulated iron oxide dust (Christensen, Philip R.,et al.).<\/p>\n

Martian soil is slightly alkaline and has traces of magnesium, sodium, potassium, and chlorine. These are elements found on Earth and are employed for the growth of vegetation (BBC News<\/em>). In addition, the soil on Mars has a pH of 7.7, and has 0.6% of salt perchlorate (Chang, Alicia). <\/p>\n

Because of atmospheric pressure, unfortunately liquid water cannot exist on the Red Planet (NASA<\/em>). There are two polar ice caps on Mars, which are mostly composed of water. Ice water is hypothesized to be trapped within the cryosphere of the planet (ESA). However, there is evidence that liquid water once existed on Mars, and that there could be liquid water in the future (\u201cMineral in Mars \u2018Berries\u2019 Adds to Water Story\u201d). <\/p>\n

In 1810, the first maps of Mars\u2019 geography was made by Johann Heinrich M\u00e4dler, which synthesized ten years of observations.<\/strong> The markings on the original map were only single letters as abbreviations for full names (Sheehan, William). Currently, many languages and names accompany maps of Mars, with the general features of Mars described by classical mythology, craters being named after deceased scientists, and even towns and cities. Valleys are either named after \u201cMars\u201d or \u201cstar\u201d in numerous languages, or named after rivers (Planetary Names<\/em>). <\/p>\n

Let us look into its atmosphere. Approximately, four billion years ago, Mars lost its magnetosphere most likely because of asteroid strikes (Wired). Due to this, solar winds directly influence the planet\u2019s ionosphere, which lowers atmospheric density. In terms of percentages, 96% of it is carbon dioxide, 1.9% argon, 1.8% nitrogen, with very little oxygen and water (Williams, David R.).<\/p>\n

Mars is often called a sister planet to Earth because of its climate, which has Earth-like seasons. <\/strong>This similarity is due to the tilts of both planets on their rotational axes. However, the lengths of the seasons on Mars are twice as long, because Mars is a greater distance from the Sun than Earth. Though Mars has extreme low temperatures, it has also has a degree of comfortable temperatures for human life. However, Mars has the largest dust storms in the galaxy, so living on Mars would not be that easy (Discover Magazine<\/em>).<\/p>\n

The Red Planet has a strange orbit. According to Universe Today<\/em>, \u201cMars\u2019 average distance (semi-major axis) from the Sun is 227,939,200 km (141,634,852.46 mi) which is roughly one and half times the distance between Earth and the Sun (1.52 AU). Compared to Earth, its orbit is also rather eccentric (0.0934 vs. 0.0167), ranging from 206.7 million km (128,437,425.435 mi; 1.3814 AU) at perihelion to 249.2 million km (154,845,701 mi; 1.666 AU) at aphelion. At this distance, and with an orbital speed of 24.077 km\/s, Mars takes 686.971 Earth days, the equivalent of 1.88 Earth years, to complete a orbit around the Sun\u201d (\u201cThe Orbit of Mars. How Long Is a Year on Mars?\u201d). This makes Mars difficult to monitor in terms of its orbit.<\/p>\n

The most pressing question about Mars is whether or not it is habitable. According to The Planetary Society<\/em>, \u201cLong-term habitation on Mars will require us to master the conversion of raw Martian materials into resources we can use to survive. Fortunately, Mars has a wealth of these materials, making it arguably the most human-habitable place in the solar system, other than the Earth itself\u201d (The Planetary Society Blog). The aspects of Mars that seems appealing to scientists in terms of its habitability is \u201catmospheric CO2, atmospheric N2 and argon, H2O from the atmosphere and polar ice, perchlorates in the regolith, nitrates in the regolith, basaltic rocks, and fluorine\u201d (The Planetary Society Blog).<\/p>\n

With this technical information in mind, we can see Mars with a much clearer mind. We can understand why Mars is favored as the next place for humans to live: it has similar seasons, it has an untapped potential in the form of ice water, and with the right technology, we can live there unperturbed. Within the next 50 years, it may be possible that the first colonies on the Red Planet will crop up.<\/p>\n

References<\/h2>\n

Zubrin, Robert; Wagner, Richard (1997). The Case for Mars: The Plan to Settle the Red Planet and Why We Must<\/em>. New York: Touchstone. ISBN 978-0-684-83550-1. OCLC 489144963.<\/p>\n

Williams, David R. (September 1, 2004). \u201cMars Fact Sheet.\u201d National Space Science Data Center. NASA<\/em>. Retrieved June 24, 2006.<\/p>\n

Nimmo, Francis; Tanaka, Ken (2005). \u201cEarly Crustal Evolution Of Mars.\u201d Annual Review of Earth and Planetary Sciences<\/em>. 33 (1): 133\u2013161. Bibcode:2005AREPS..33..133N. doi:10.1146\/annurev.earth.33.092203.122637.<\/p>\n

Rivoldini, A.; Van Hoolst, T.; Verhoeven, O.; Mocquet, A.; Dehant, V. (June 2011). \u201cGeodesy constraints on the interior structure and composition of Mars.\u201d Icarus<\/em>. 213 (2): 451\u2013472. Bibcode:2011Icar..213..451R. doi:10.1016\/j.icarus.2011.03.024.<\/p>\n

Jacqu\u00e9, Dave (September 26, 2003). \u201cAPS X-rays reveal secrets of Mars\u2019 core.\u201d Argonne National Laboratory<\/em>. Archived from the original on February 21, 2009. Retrieved July 1, 2006.<\/p>\n

McSween, Harry Y.; Taylor, G. Jeffrey; Wyatt, Michael B. (May 2009). \u201cElemental Composition of the Martian Crust.\u201d Science<\/em>. 324 (5928): 736\u2013739. Bibcode:2009Sci\u2026324..736M. doi:10.1126\/science.1165871. PMID 19423810.<\/p>\n

Christensen, Philip R.; et al. (June 27, 2003). \u201cMorphology and Composition of the Surface of Mars: Mars Odyssey THEMIS Results.\u201d Science. 300(5628): 2056\u20132061. Bibcode:2003Sci\u2026300.2056C. doi:10.1126\/science.1080885. PMID 12791998.<\/p>\n

\u201cMartian soil \u2018could support life.\u201d\u2019 BBC News<\/em>. June 27, 2008. Retrieved August 7, 2008.<\/p>\n

Chang, Alicia (August 5, 2008). \u201cScientists: Salt in Mars soil not bad for life.\u201d USA Today<\/em>. Associated Press. Retrieved August 7, 2008.<\/p>\n

\u201cNASA \u2013 NASA Rover Finds Clues to Changes in Mars\u2019 Atmosphere.\u201d NASA<\/em>.<\/p>\n

\u201cWater ice in crater at Martian north pole.\u201d ESA<\/em>. July 28, 2005. Retrieved March 19, 2010.<\/p>\n

\u201cMineral in Mars \u2018Berries\u2019 Adds to Water Story\u201d (Press release). NASA<\/em>. March 3, 2004. Archived from the original on November 9, 2007. Retrieved June 13, 2006.<\/p>\n

Sheehan, William. \u201cAreographers.\u201d The Planet Mars: A History of Observation and Discovery<\/em>. Retrieved June 13, 2006.<\/p>\n

Planetary Names: Categories for Naming Features on Planets and Satellites. Planetarynames.wr.usgs.gov<\/em>. Retrieved December 1, 2011.<\/p>\n

\u201cMultiple Asteroid Strikes May Have Killed Mars\u2019s Magnetic Field.\u201d Wired<\/em>. January 20, 2011.<\/p>\n

Kluger, Jeffrey (September 1, 1992). \u201cMars, in Earth\u2019s Image.\u201d Discover Magazine<\/em>. Retrieved November 3, 2009.<\/p>\n

\u201cThe Orbit of Mars. How Long Is a Year on Mars?\u201d Universe Today<\/em>, 17 Apr. 2017, www.universetoday.com\/14718\/how-long-is-a-year-on-mars\/.<\/p>\n

\u201cIs Mars Habitable? With the Right Technologies, Yes.\u201d The Planetary Society Blog<\/em>, www.planetary.org\/blogs\/guest-blogs\/2017\/20170921-mars-isru-tech.html.<\/p>\n<\/p><\/div>\n","protected":false},"excerpt":{"rendered":"

Mars is featured in countless science-fiction books, non-fiction books, cartoons, films, and more. However, how much do we know about the Red Planet? I would say that the average person only has a cursory knowledge of this important part of Read More …<\/a><\/p>\n","protected":false},"author":1,"featured_media":24122,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[39,17,40,41,42],"tags":[],"class_list":["post-436059","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-academic-articles-assignment-help","category-academic-assignment-help","category-academic-assignments","category-academic-essay-writing-uk","category-academic-essays-help"],"_links":{"self":[{"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/posts\/436059","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/comments?post=436059"}],"version-history":[{"count":0,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/posts\/436059\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/posts\/24122"}],"wp:attachment":[{"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/media?parent=436059"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/categories?post=436059"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.benedictsol.com\/blogs\/wp-json\/wp\/v2\/tags?post=436059"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}