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The Cosmological Risks Surrounding the Planet Earth and the Extent of Actuaries Tracking

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The planet Earth is exposed to various external risks; perhaps the most important of them at the present time are magnetic storms that originate from the sun and meteorites of multiple sizes that collide with the Earth over time. This paper discusses these two phenomena and assesses their impact on the planet Earth.
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The Sciences: Cosmology:
The Cosmological Risks Surrounding
the Planet Earth and
the Extent of Actuaries Tracking
by Dr. Samir Ahmed Hamouda and Fatima Melad Alshareeif
Department of Physics, University of Benghazi, Benghazi, Libya
dr_s_hamouda@yahoo.ie
Link for Citation Purposes: https://bwwsociety.org/journal/current/2021/may-jun/the-
cosmolgical-risks-the-planet-earth.htm
Abstract:
The planet Earth is exposed to various external risks; perhaps the most important of them at the
present time are magnetic storms that originate from the sun and meteorites of multiple sizes
that collide with the Earth over time. This paper discusses these two phenomena and assesses
their impact on the planet Earth.
Keywords: Solar System, Meteorites, Magnetic Storms, Earth Risks, Asteroid Belt.
1. Introduction:
The solar system contains eight planets with their moons and many objects that deserve
attention such as comets, meteors and asteroids, where the sun constitutes approximately
99.85% of the mass of the group while the other planets represent the rest percentage as shown
in figure 1. Due to the force of solar gravity, each planet retains an almost circular orbit and
revolves around the sun in a counterclockwise direction and about different axis orientations.
Figure 1: The solar system [1].
2. The Solar Activity
The sun is the first source that threatens human life on the surface of the earth due to its great
impact on economic, health activities, and human behavior. Such impacts come from sunspots
activity. The importance of studying this topic lies in the consideration that many scientists
believe that sunspots activity have a direct relationship to human life on Earth. There are many
theories, interpretations, and statistics through which scientists try to find connections between
sunspots activity, health activity, economic, agricultural, and human behavior. On the other
hand, some scientists also believe that global warming is due to reasons of human activities,
although the real causes of this phenomenon are not yet known. Preliminary studies on this
phenomenon have shown that global climate change is not only a ground phenomenon but also
due to solar system activity. The generation mechanisms of the sunspots are explained
elsewhere [2].
In a recent case, Earth-orbiting satellites detected the strongest magnetic storm resulting from a
solar flare and Coronal Mass Ejection (CME) event. Figure 2 illustrates the size of the CME
shockwave edge with respect to the size of the sun at the point of the outburst. The eruption that
produced this flare also sent a solar rippling through the sun’s atmosphere and ejected a CME
toward Earth. By the time the CME reached the Earth, the shockwave leading edge had
expanded to approximately 40 million miles across [3].
Figure 2: Solar flare and coronal mass ejection at the time of the eruption [3].
Additionally, eruptive and transient phenomena in the sun/corona and in the interplanetary
medium can lead to the acceleration of energetic particles with greatly enhanced flux. Such
processes can modify the radiation environment on Earth and need to be taken into account for
planning and maintaining space missions. Solar activity can cause, through coupling of solar
wind and the Earth’s magnetosphere, strong geomagnetic storms in the magnetosphere and
ionosphere, which may disturb radio-wave propagation and navigation-system stability, or
induce dangerous spurious currents in long pipes or power lines. Another important aspect is
the link between solar-activity variations and the Earth’s climate [4]. These changes have a
great impact on the terrestrial environment and on many aspects of human lives. Therefore,
studying and modeling solar activity can increase the level in demand to understanding of
nature.
It is important to study solar variability on different timescales. The behavior of solar activity in
the past (see figure3.) is of great importance for a variety of reasons:
Figure 3: Sunspot observations on different timescales [5]
(i) It allows an improved knowledge of the statistical behavior of the solar-dynamo process,
which generates the cyclically varying solar-magnetic field. (ii) Making it possible to estimate
the fractions of time the sun spends in states of very-low activity called grand minima. Such
studies require a long time series of solar activity data. The longest direct series of solar activity
is the 400-year-long sunspot-number series, which depicts the dramatic contrast between the
(almost spotless) Maunder minimum and the modern period of very high activity. This allows
one to study the temporal evolution of solar magnetic activity, and thus of the solar dynamo, on
much longer timescales than are available from direct measurements [4]. Although sunspots
have been extensively studied for almost 400 years and their magnetic nature has been known
since 1908, gaining the knowledge about their basic properties is still evolving [6].
During the Maunder Minimum periods of low solar sunspot activity, there was also an increase
in the ratio of radio-carbon 14 (14C to 12C) in tree rings and there were documented changes in
the aurora borealis. Each of these periods was known for bitterly cold and prolonged winters in
the Northern Hemisphere. The Maunder Minimum occurred during most of the 17th Century
and the first decade of the 18th Century [7]. A later period of relatively low sunspot activity
commenced in the last two decades of the 18th Century and lasted for the first three decades of
the 19th Century. This period is known as the Dalton Minimum. The two grand minima were
collectively called the (Little Ice-Age) [7].
Many studies have suggested the sunspot activity influences on Nature’s Risks, and explain
how the decreased levels of sunspot activity will affect long-term weather risks as well as long-
term earthquake and volcanic risks [7]. The aim of these studies is to encourage the actuarial
profession to develop skills in space weather forecasting and understand the risk management
activities that arise from such abilities. Also to understand why, at certain times, when solar
flares that hit Earth, they have the ability to temporarily significantly change climatic
conditions, earthquake and volcanic risks. Understanding just these mechanisms should
convince the profession to develop important real-time risk management tools and capabilities
that can be applied in many areas of expertise as well as in new areas where actuaries where
actuaries are unaware of. Understanding how natural forces (in particular the current prolonged
low sunspot activity of the sun) affect a number of risks that should interest actuaries. These
include human mortality, natural events such as major earthquakes and volcanic eruptions,
direct weather related risks, in particular, from weather extremes [7].
Other category of risks that are important, include risks relating to food and energy security, the
political risks arising from unaffordable increases in the price of these commodities, crop
insurance and other forms of insurance that are affected by climatic extremes. Understanding
the sun-climate connection requires a breadth of expertise in fields such as solar activity, plasma
physics, energetic particle physics, atmospheric chemistry, fluid dynamics, and even terrestrial
history. However, researchers are asked to have the full range of knowledge required to solve
the sun-climate connection problem.
3. Asteroid Belt
The second threat to life on Earth's surface is the existence of the Asteroid Belt in the solar
system. Asteroid Belt is different sized bodies believed to have been remained since the
formation of the solar system 4.6 billion years ago. They are rocky bodies of irregular shapes,
and most of them are small in size. The asteroid belt lies in an area between Mars and Jupiter
and is called the main belt (see figure 4.).
Figure 4: The Asteroid Belt [8].
Planet Ceres is one of the largest bodies in this belt, as it represents about 25% of the mass of
the belt, followed by asteroids Pallas, Hygiea, and Vesta, represent about half the mass of this
belt. Asteroids Belt ranges in size from Ceres as its largest body to grains like dust particles.
Most asteroids are irregularly shaped, but some are nearly spherical and often contain craters.
The asteroids orbit in elliptical orbits around the sun, and they also revolve around themselves,
in irregular rotations [9].
3.1 Source of Meteorites
While the asteroid belt is considered the most probable source of meteorite origin, some
meteorites have chemical structures similar to samples collected from the surface of the moon,
(where Allan Hills 81005 is the first meteorite from the origin of the moon) and others believe
that it came from Mars due to collisions of other asteroids or from The path of volcanic
eruptions on its surface. Records from the past time have shown that large meteorites cause
tremendous damage to the planet Earth and to life on it. A collision of a large meteorite with the
earth may lead to the generation of a crater with a diameter of 10-20 km, at about twice its
diameter. Such meteorite impacts with the planet Earth lead to the generation of a force
equivalent to the force of an explosion between one nuclear bomb to thousands of nuclear
bombs (see figure 5).
Figure 5: The frequency of meteorites colliding with Earth
and its relationship to meteorite size [10]
The force generated by the collision varies according to the size and speed of the meteorite, for
example: the force of the Siberian meteorite explosion in 1908 was 1,000 times stronger than
the Hiroshima bomb. Figure 6, shows some of the meteorite collision sites with the Earth [11].
Figure 6: The density of meteorites fall on continents [11].
Figure 7, shows the Vredefort crater, with an estimated diameter of 300 kilometers, is the
world's largest known impact structure. It was created when an asteroid measuring at least 10
kilometers landed on Earth an estimated 2 billion years ago.
Figure 7: The Vredefort crater [12]
However, solutions to prevent meteorites colliding with the Earth are suggested: (i) Destruction
of a meteorite from one side outside the Earth's airspace by using nuclear missiles, which could
deflect the meteor's path away from the Earth. (ii) The attempt to propel the jet, which is based
on sending a vehicle to the meteorite to join with it and try to change its path. (iii) The meteorite
was pushed by gravity by sending a very huge vehicle that moves in parallel with the meteor,
and as a result of its speed, gravity produces a slight movement of the meteor, causing it to
derail its path.
The subject of meteorites at the global level is of great scientific and environmental importance,
and this importance lies in the field of space physics, through which the components of
meteorites are studied, which reflect the components of the solar system when it was formed.
The other importance is an environmental importance that is directly related to the future of
human civilization due to the violent destructive phenomena they cause on Earth and this
requires studying the mechanics of meteorites colliding with Earth and estimate the extent of
the devastation they are causing on the surface of the earth [13-18].
4. Conclusion
Understanding the solar system cycle remains the main problem in solar physics. Although
sunspots activity has been extensively studied for almost 400 years and their magnetic nature
has been known since 1908, our knowledge about their basic properties is still evolving.
Climate change on the planet is presently one of the most controversial debates among experts
and scientists. Some scientists believe that global warming is due to reasons of human actions,
although the real causes of this phenomenon are not yet known. However, lead-in studies on
this phenomenon have shown that global climate change is also connected to sunspots activity.
The subject of space physics is one of the most important topics in the field of scientific
research, which enjoys global attention and gives distinctive value to the leading universities in
research capabilities and the number of scientific publications related to this field. Among the
important topics in the field of space physics is the subject of meteorites. Meteorites are
remnants resulting from the formation of the solar system, the study of meteorites, allows
identifying the chemical compositions of the solar system when it was formed as well as
estimating the extent of the devastation they are causing on the surface of the earth and to find
Possible solutions to prevent their collision with the Earth.
References:
[1] Solar System photos - Google
Search
[2] Samir A Hamouda et al. (2018),” Sunspots Production and Relation to Other Phenomena: A
Review, International Journal of science and research methodology; Vol. 9 (4): 141-158[3] ICS-
CERT ADVISORY., (2011).
[3] “SOLAR MAGNETIC STORM IMPACT ON CONTROL SYSTEMS”.,ICS-CERT.,
https://ics-cert.us-cert.gov/advisories/ICSA-11-084-01
[4] Ilya G. Usoskin, (2008) “A History of Solar Activity over Millennia”., Living Rev. Solar
Phys. http://www.livingreviews.org/lrsp-2008-3
[5] Rachel MacDonald. et. al. (2006)., “What's a Sunspot?”, TJO News., The Theodor Jacobsen
Observatory
Newsletter.http://www.devinsilvia.com/publications/tjo_au06win07.pdf
[6] Sami K. Solanki, (2003)., “Sunspots: An overview”, The Astron Astrophys Rev. 11: 153–
286
[7] Brent Walker, (2013)., The New Grand Minimum”., Institute of Actuaries of
Australia.,https://www.actuaries.asn.au/Library/Events/SUM/2013/Sum2013PaperBrentWalker.
pdf
[8] Main Asteroid Belt | COSMOS
(swin.edu.au)
[9]
http://www.daviddarling.info/encyclopedia/A/asteroid.html
[10]
http://www.tulane.edu/~sanelson/Natural_Disasters/impacts.htm
[11] Earth Impact Database,
http://www.passc.net/EarthImpactDatabase/Namesort.html
[12] vredefort photo - Google
Search
[13] G. A. EIBY., “A Survey of the Tektite Problem ”., New Zealand Journal of Geology and
Geophysics ., 2., 1959., 183-94.
[14] G. J. Taylor., Gamma Rays, Meteorites, Lunar Samples, and the Composition of the
Moon”., Planetary Science Research Discoveries., (2005):
http://www.psrd.hawaii.edu/Nov05/MoonComposition.html
[15] R. L. Korotev et al., “ Compositions of three lunar meteorites: Meteorite Hill 01210,
Northeast Africa 001,and Northwest Africa 3136”., Lunar and Planetary Science XXXVI.,
(2005)., Abstract # 1220
[16] R. L. Korotev., “ Composition of Lynch 002 Lunar Meteorite”., 76th Annual Meteoritic
Society Meeting., (2013)., Abs.
5021
[17] A. Wittmann et al., “ Trace Elements Composition of Impact Melts In Lunar Meteorite
Shisr 161”., 76Th Annual Meteoritic Society Meeting., (2013)., Abstract #
5262
[18] L. R. Nittler et al., “Bulk element compositions of meteorites: a guide for interpreting
remote-sensing geochemical measurements of planets and asteroids”, Antarct. Meteorite Res.,
17, (2004), 233-253
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Composition of Lynch 002 Lunar Meteorite
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