The document discusses the atmosphere and its interactions with Earth's other systems. It makes the following key points:
1) The sun's radiation warms Earth's systems at different rates, creating wind and ocean currents.
2) The early atmosphere was mainly the result of gases from volcanoes. Life and the atmosphere have evolved together.
3) For hundreds of millions of years, the atmosphere composition has remained stable due to interactions with the hydrosphere, biosphere, and geosphere.
Are you curious about how universe began? well, we are willing to share our knowledge about this! by the help of this site.
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Planet Earth and its properties necessary to support lifeSimple ABbieC
Department of Education | Senior High School
Topic: Planet Earth and its properties necessary to support life.
Learning Competency:
Earth and Life Science: Recognize the uniqueness of Earth, being the only planet in the Solar System with properties necessary to support life.
Earth Science (for STEM): Describe the characteristics of Earth that are necessary to support life.
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Are you curious about how universe began? well, we are willing to share our knowledge about this! by the help of this site.
Welcome to our website!
We will assure you that you will learn a lot!
Enjoy and have a great day!
Planet Earth and its properties necessary to support lifeSimple ABbieC
Department of Education | Senior High School
Topic: Planet Earth and its properties necessary to support life.
Learning Competency:
Earth and Life Science: Recognize the uniqueness of Earth, being the only planet in the Solar System with properties necessary to support life.
Earth Science (for STEM): Describe the characteristics of Earth that are necessary to support life.
Please LIKE / FOLLOW and SHARE my other social media accounts.
Facebook: https://www.facebook.com/Simple-ABbieC-131584525051378/
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Youtube:
http://tiny.cc/SimpleABbieC
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Slideshare:
https://www.slideshare.net/AbbieMahinay
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Blogger:
https://simpleabbiec.blogspot.com/?m=1
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the Earth and its Subsystems (The Four Spheres).
"Plants on Other Planets May Not be Green" presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway
Earth Science (Kebumian) Material with Double Language (Bahasa-English)
this material only for Secondary High School Learning or for people want to teach earth science
This is a powerpoint presentation that is about one of the Senior High School Core Subject: Earth and Life Science. It is composed of the theories that explains the Earth and its Subsystems (The Four Spheres).
"Plants on Other Planets May Not be Green" presentation was given during a Journal-Club meeting on 30th of April 2007 at National University of Ireland, Galway
Earth Science (Kebumian) Material with Double Language (Bahasa-English)
this material only for Secondary High School Learning or for people want to teach earth science
The future life span of Earth’s oxygenated atmosphereSérgio Sacani
Earth’s modern atmosphere is highly oxygenated and is a remotely detectable signal of
its surface biosphere. However, the lifespan of oxygen-based biosignatures in Earth’s
atmosphere remains uncertain, particularly for the distant future. Here we use a
combined biogeochemistry and climate model to examine the likely timescale of
oxygen-rich atmospheric conditions on Earth. Using a stochastic approach, we find that
the mean future lifespan of Earth’s atmosphere, with oxygen levels more than 1% of the
present atmospheric level, is 1.08 ± 0.14 billion years (1σ). The model projects that a
deoxygenation of the atmosphere, with atmospheric O2 dropping sharply to levels
reminiscent of the Archaean Earth, will most probably be triggered before the inception
of moist greenhouse conditions in Earth’s climate system and before the extensive loss
of surface water from the atmosphere. We find that future deoxygenation is an
inevitable consequence of increasing solar fluxes, whereas its precise timing is
modulated by the exchange flux of reducing power between the mantle and the ocean–
atmosphere–crust system. Our results suggest that the planetary carbonate–silicate cycle
will tend to lead to terminally CO2-limited biospheres and rapid atmospheric
deoxygenation, emphasizing the need for robust atmospheric biosignatures applicable
to weakly oxygenated and anoxic exoplanet atmospheres and highlighting the potential
importance of atmospheric organic haze during the terminal stages of planetary
habitability.
The Oxygen Bottleneck for TechnospheresSérgio Sacani
On Earth, the development of technology required easy access to open air combustion, which is only possible when oxygen partial pressure, P(O2), is above
18%. This suggests that only planets with significant atmospheric concentrations
will be capable of developing “advanced” technospheres and hence detectable
technosignatures.
Proposing the use of a global probe based network of durable marine “laborato...Hofstra University
This was my final project for my sedimentary geology class. The task was to come up with an original research project that was based on a topic relevant to the environment.
What are some of the basic principles and terminology involved in climate change? Learn more about the Earth's atmosphere, energy balance, and how the greenhouse effect can alter both climate and weather. What is climate forcing? What is climate feedback? For more on this topic, visit: http://extension.org/60702
Similar to Kisi-kisi Eso day 3 (Atmosphere and ES) (20)
Earth Science (Kebumian) Material with the English Language
this material only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material with Double Language (Bahasa-English)
this material only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material with Double Language (Bahasa-English)
this material only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material with Bahasa Indonesia
this material only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material Bahasa Indonesia version
this material only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material with English Language
this is Sedimentary ROck Environment only for Secondary High School Learning or for people want to teach earth science
Earth Science (Kebumian) Material with Double Language (Bahasa-English)
this is Basic Litosphere only for Secondary High School Learning or for people want to teach earth science
Feel Free to contact me for learn regarding Earth Science (Kebumian)
This Powerpoint for Indonesian's Students with Based Curriculum and double language (Bahasa-English)
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
A brief information about the SCOP protein database used in bioinformatics.
The Structural Classification of Proteins (SCOP) database is a comprehensive and authoritative resource for the structural and evolutionary relationships of proteins. It provides a detailed and curated classification of protein structures, grouping them into families, superfamilies, and folds based on their structural and sequence similarities.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Multi-source connectivity as the driver of solar wind variability in the heli...Sérgio Sacani
The ambient solar wind that flls the heliosphere originates from multiple
sources in the solar corona and is highly structured. It is often described
as high-speed, relatively homogeneous, plasma streams from coronal
holes and slow-speed, highly variable, streams whose source regions are
under debate. A key goal of ESA/NASA’s Solar Orbiter mission is to identify
solar wind sources and understand what drives the complexity seen in the
heliosphere. By combining magnetic feld modelling and spectroscopic
techniques with high-resolution observations and measurements, we show
that the solar wind variability detected in situ by Solar Orbiter in March
2022 is driven by spatio-temporal changes in the magnetic connectivity to
multiple sources in the solar atmosphere. The magnetic feld footpoints
connected to the spacecraft moved from the boundaries of a coronal hole
to one active region (12961) and then across to another region (12957). This
is refected in the in situ measurements, which show the transition from fast
to highly Alfvénic then to slow solar wind that is disrupted by the arrival of
a coronal mass ejection. Our results describe solar wind variability at 0.5 au
but are applicable to near-Earth observatories.
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
3. Semua orang HARUS punya tujuan,
Semua orang punya KAPASITAS OTAK yang sama,
Tidak ada Kata Terlambat,
Bermimpilah melebihi GURU MU
Siapa yang tidak suka?
6. Key ideas
ATMOSPHERE IMPACTS
1. The radiation from the sun causes warming (1) of
all of Earth systems, but the rate of absorbing and
radiation of heat in rocks (Geosphere), water
(Hydrosphere) and air (Atmosphere) varies from
one to the other. This phenomenon creates, at the
end of a complex process, local and global flow
systems (2) in the Atmosphere (wind) and oceans.
Isu – isu terbaru dunia kebumian
7. HISTORY ATMOSPHERE
2. The composition of the primary atmosphere
of earth (3) was mainly the result of gasses that
were emitted by volcanoes. The evolution of the
atmosphere is intertwined with the evolution of
life on Earth.
8. ATMOSPHERE RELATIONS
3. For hundreds of millions of years the
atmosphere keeps a more or less similar
composition as a result of the mutual relations
among the atmosphere with the hydrosphere
(oceans) (4), biosphere (photosynthesis and
breathing (5)) and the geosphere (gas, volcanic
dust and erosion (6)).
9. HUMAN ACTION IMPACTS
4. In the short term human actions cause
minimal imbalance in the atmosphere (7), but
in the long term the oceans will become huge
sinks that regulate part of the atmosphere
composition. Since the biosphere is affected in
the short term, even minute and temporary
changes can cause terminal changes to part of
the biosphere.
10. b) Skills and
Abilities
1. The ability to distinguish between the
components of a geochemical system (8), to
identify mutual relations (9) and to construct a
network of interactions among them (10).
2. The ability to identify the interactions between
the parts of the system as dynamic processes of
matter and energy (11).
3. The ability to identify environmental problems
and suggest solutions (12) on the basis of
understanding the principles of the
geobiochemical system.
12. TUGAS
1. Answer Search Reasons (ASR), soal soal yang
tadi di ASR-in, besok WAJIB dikumpul.
2. Jawab analisis gambar di IG melalui
komentar: @ronimarudut