Microbes are tiny organisms that can only be seen with a microscope. They are found everywhere in the environment and inside and on humans and animals. While most microbes are harmless or beneficial, some can cause illness. There are more microbes on the human body and in soil and oceans than any other type of organism. The three main types of microbes are bacteria, viruses, and fungi. Microbes play a vital role in ecosystems by decomposing waste, generating oxygen, and participating in nutrient cycles. They also aid in food production and help break down food in human and animal digestive systems.
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micro, microorganism, friend , foe, science , activity, 8th class
types of microorganism
types of bacteria
fungus protozoa
algae
viruses
diseases
you will learn about
1 What is microorganisms' .
2.types of microorganisms' .
3 .Advantages and Disadvantages of microorganisms' .
4. Examples of microorganisms' .
5. microorganism on microscope .
Thank you .
General introduction to micro organisms. What are micro-organisms? Microorganism. Bacteria, viruses, fungi, algae, protozoans, Microbiology, father of microbiology, PowerPoint Presentation.
comment if you like it
micro, microorganism, friend , foe, science , activity, 8th class
types of microorganism
types of bacteria
fungus protozoa
algae
viruses
diseases
you will learn about
1 What is microorganisms' .
2.types of microorganisms' .
3 .Advantages and Disadvantages of microorganisms' .
4. Examples of microorganisms' .
5. microorganism on microscope .
Thank you .
General introduction to micro organisms. What are micro-organisms? Microorganism. Bacteria, viruses, fungi, algae, protozoans, Microbiology, father of microbiology, PowerPoint Presentation.
In the presentation I have shown the various ways the microbes help us in our day to day life. There are different types of microbes in and around us who help us in ways we even don't know about. Please comment if any improvement needed.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
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THE IMPORTANCE OF MARTIAN ATMOSPHERE SAMPLE RETURN.Sérgio Sacani
The return of a sample of near-surface atmosphere from Mars would facilitate answers to several first-order science questions surrounding the formation and evolution of the planet. One of the important aspects of terrestrial planet formation in general is the role that primary atmospheres played in influencing the chemistry and structure of the planets and their antecedents. Studies of the martian atmosphere can be used to investigate the role of a primary atmosphere in its history. Atmosphere samples would also inform our understanding of the near-surface chemistry of the planet, and ultimately the prospects for life. High-precision isotopic analyses of constituent gases are needed to address these questions, requiring that the analyses are made on returned samples rather than in situ.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
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.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
(May 29th, 2024) Advancements in Intravital Microscopy- Insights for Preclini...Scintica Instrumentation
Intravital microscopy (IVM) is a powerful tool utilized to study cellular behavior over time and space in vivo. Much of our understanding of cell biology has been accomplished using various in vitro and ex vivo methods; however, these studies do not necessarily reflect the natural dynamics of biological processes. Unlike traditional cell culture or fixed tissue imaging, IVM allows for the ultra-fast high-resolution imaging of cellular processes over time and space and were studied in its natural environment. Real-time visualization of biological processes in the context of an intact organism helps maintain physiological relevance and provide insights into the progression of disease, response to treatments or developmental processes.
In this webinar we give an overview of advanced applications of the IVM system in preclinical research. IVIM technology is a provider of all-in-one intravital microscopy systems and solutions optimized for in vivo imaging of live animal models at sub-micron resolution. The system’s unique features and user-friendly software enables researchers to probe fast dynamic biological processes such as immune cell tracking, cell-cell interaction as well as vascularization and tumor metastasis with exceptional detail. This webinar will also give an overview of IVM being utilized in drug development, offering a view into the intricate interaction between drugs/nanoparticles and tissues in vivo and allows for the evaluation of therapeutic intervention in a variety of tissues and organs. This interdisciplinary collaboration continues to drive the advancements of novel therapeutic strategies.
2. Microbes
• Are invisible to the naked eye, you need a
powerful microscope to see them.
• Are everywhere around us, inside us, on
us, in our food, in our homes, in the air we
breathe and the water we wash in.
• Are mostly useful, but some are harmful
• Have been around for 3.8 bn years.
• Are vital for life on Earth.
3. What do Microbes look like ?
Magnified 1000s of times and colored using
dye, we see -
4. Microbes exist in huge numbers
In one single teaspoon of garden soil, there are
over 100,000 microbes. In 1ltr of seawater, there
are over 1bn microbes.
On your hands there are more microbes than there
are people in the world.
There are so many microbes, that scientists have
only named 0.5% of them.
Microbes outnumber all other species and make
up most of the living matter on the planet.
6. Bacteria
• Have three main shapes
spira l(boriella) little balls(-cocci) rods (-bacilli)
• Can move about on their own
• Join up together to form chains
called ‘bio-films’. As on teeth !
7. What can bacteria do ?
Bacteria in the Cafeteria - lets find out using this
webpage.
We have learned that bacteria do many good
things, such as decompose waste and give
texture and flavor to food. However, they can
also cause illness. They give off oxygen when
they ‘eat’. Half of all the oxygen in the world,
comes from bacteria.
8. Virus
Come in 1000s of different shapes and sizes.
They hang about waiting to meet a ‘host’ which
they then invade, hijacking the host’s cells.
Beware the air you breathe and door handles !
10. Algae are also Microbes
• Algae photosynthesize – taking their
energy from the sun, and producing
oxygen in the process. Algae are thought
to produce over 50% of the oxygen in the
world.
11. Microbes live among us
• In our food
• Cleaning up our waste
• Killing pests
• Making medicines
• In the making of such things as leather,
soy sauce, cheese and paper.
• In our bodies. Microbes in
our mouths
12. And finally
• Without microbes, life on this planet would be
entirely different – they generate oxygen, are
part of the carbon and nitrogen cycles, and can
survive the harshest conditions.
• Without microbes, our bodies would not process
the food we eat.
• They drive the chemistry of life, breaking things
down into their parts so that life can being again.
• Microbes are small but mighty !
13. To find out more
• www.microbe.org
• www.amnh.org/exhibitions/epidemic
• www.mikeymicrobe.com
• www.cellsalive.com/howbig