Photosynthesis converts sunlight, water and carbon dioxide into oxygen and energy in the form of ATP and NADPH. It takes place in chloroplasts and involves two stages: the light-dependent reactions capture energy from sunlight to produce ATP and NADPH, while the carbon fixation reactions use these products to incorporate CO2 into organic molecules like glucose. Many scientists contributed to discovering the process of photosynthesis, including how water is the source of oxygen produced.
In this ppt, you will learn about photosystem first of photosynthesis, with video and animation such a nice presentation. electron movement by animation, see and understand the system.
This presentation describes in details how photosynthesis works along with its process. It also explains in details on the light-dependent and light-independent reactions.
In this ppt, you will learn about photosystem first of photosynthesis, with video and animation such a nice presentation. electron movement by animation, see and understand the system.
This presentation describes in details how photosynthesis works along with its process. It also explains in details on the light-dependent and light-independent reactions.
Photosynthesis (Light and Dark reaction of photosynthesis)Shekhar Tidke
Importance of photosynthesis. Light reaction of photosynthesis, Dark reaction of photosynthesis. Hill, and Blackman reaction or C3 cycle or Calvin Cycle
Photosynthesis has two types of reaction, first one is light reaction (Hill's reaction) and the other one is dark reaction (Blackman's reaction). In this presentation you learn full mechanism of how plants produce energy for their survival by photosynthesis.
Photosynthesis is a process used by plants and other organisms to convert light energy, normally from the sun, into chemical energy that can be used to fuel the organisms' activities. Carbohydrates, such as sugars, are synthesized from carbon dioxide and water.
Photosynthesis (Light and Dark reaction of photosynthesis)Shekhar Tidke
Importance of photosynthesis. Light reaction of photosynthesis, Dark reaction of photosynthesis. Hill, and Blackman reaction or C3 cycle or Calvin Cycle
Photosynthesis has two types of reaction, first one is light reaction (Hill's reaction) and the other one is dark reaction (Blackman's reaction). In this presentation you learn full mechanism of how plants produce energy for their survival by photosynthesis.
Photosynthesis is a process used by plants and other organisms to convert light energy, normally from the sun, into chemical energy that can be used to fuel the organisms' activities. Carbohydrates, such as sugars, are synthesized from carbon dioxide and water.
Geological Evidence for photosynthesis, mechanisms of evolution, evolution of co-factors, evolution of protein complexes, photosynthetic reaction centers and electron transport chains
Khảo sát thành phần hóa học cao methanol trong lá cây chùm ngây moringa oleif...NOT
Giá 10k/lượt download Liên hệ page để mua: https://www.facebook.com/garmentspace Xin chào, Nếu bạn cần mua tài liệu xin vui lòng liên hệ facebook: https://www.facebook.com/garmentspace Tại sao tài liệu lại có phí ??? Tài liệu một phần do mình bỏ thời gian sưu tầm trên Internet, một số do mình bỏ tiền mua từ các website bán tài liệu, với chi phí chỉ 10k cho lượt download tài liệu bất kỳ bạn sẽ không tìm ra nơi nào cung cấp tài liệu với mức phí như thế, xin hãy ủng hộ Garment Space nhé, đừng ném đá. Xin cảm ơn rất nhiều
The pigment chlorophyll is found inside the chloroplasts, each leaf contains millions of chloroplasts. Inside each one, there are stacks of membranes that hold the chlorophyll molecules.
this presentation contains briefing of the chapter as per NCERT syllabus in details that contains photosynthesis process, early experiments, photosynthetic pigments,photophosphorylation, light reactions and dark reactions n factors affecting photsynthesis.
(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.
Observation of Io’s Resurfacing via Plume Deposition Using Ground-based Adapt...Sérgio Sacani
Since volcanic activity was first discovered on Io from Voyager images in 1979, changes
on Io’s surface have been monitored from both spacecraft and ground-based telescopes.
Here, we present the highest spatial resolution images of Io ever obtained from a groundbased telescope. These images, acquired by the SHARK-VIS instrument on the Large
Binocular Telescope, show evidence of a major resurfacing event on Io’s trailing hemisphere. When compared to the most recent spacecraft images, the SHARK-VIS images
show that a plume deposit from a powerful eruption at Pillan Patera has covered part
of the long-lived Pele plume deposit. Although this type of resurfacing event may be common on Io, few have been detected due to the rarity of spacecraft visits and the previously low spatial resolution available from Earth-based telescopes. The SHARK-VIS instrument ushers in a new era of high resolution imaging of Io’s surface using adaptive
optics at visible wavelengths.
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.
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Monitor common gases, weather parameters, particulates.
This pdf is about the Schizophrenia.
For more details visit on YouTube; @SELF-EXPLANATORY;
https://www.youtube.com/channel/UCAiarMZDNhe1A3Rnpr_WkzA/videos
Thanks...!
Richard's aventures in two entangled wonderlandsRichard Gill
Since the loophole-free Bell experiments of 2020 and the Nobel prizes in physics of 2022, critics of Bell's work have retreated to the fortress of super-determinism. Now, super-determinism is a derogatory word - it just means "determinism". Palmer, Hance and Hossenfelder argue that quantum mechanics and determinism are not incompatible, using a sophisticated mathematical construction based on a subtle thinning of allowed states and measurements in quantum mechanics, such that what is left appears to make Bell's argument fail, without altering the empirical predictions of quantum mechanics. I think however that it is a smoke screen, and the slogan "lost in math" comes to my mind. I will discuss some other recent disproofs of Bell's theorem using the language of causality based on causal graphs. Causal thinking is also central to law and justice. I will mention surprising connections to my work on serial killer nurse cases, in particular the Dutch case of Lucia de Berk and the current UK case of Lucy Letby.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
Introduction:
RNA interference (RNAi) or Post-Transcriptional Gene Silencing (PTGS) is an important biological process for modulating eukaryotic gene expression.
It is highly conserved process of posttranscriptional gene silencing by which double stranded RNA (dsRNA) causes sequence-specific degradation of mRNA sequences.
dsRNA-induced gene silencing (RNAi) is reported in a wide range of eukaryotes ranging from worms, insects, mammals and plants.
This process mediates resistance to both endogenous parasitic and exogenous pathogenic nucleic acids, and regulates the expression of protein-coding genes.
What are small ncRNAs?
micro RNA (miRNA)
short interfering RNA (siRNA)
Properties of small non-coding RNA:
Involved in silencing mRNA transcripts.
Called “small” because they are usually only about 21-24 nucleotides long.
Synthesized by first cutting up longer precursor sequences (like the 61nt one that Lee discovered).
Silence an mRNA by base pairing with some sequence on the mRNA.
Discovery of siRNA?
The first small RNA:
In 1993 Rosalind Lee (Victor Ambros lab) was studying a non- coding gene in C. elegans, lin-4, that was involved in silencing of another gene, lin-14, at the appropriate time in the
development of the worm C. elegans.
Two small transcripts of lin-4 (22nt and 61nt) were found to be complementary to a sequence in the 3' UTR of lin-14.
Because lin-4 encoded no protein, she deduced that it must be these transcripts that are causing the silencing by RNA-RNA interactions.
Types of RNAi ( non coding RNA)
MiRNA
Length (23-25 nt)
Trans acting
Binds with target MRNA in mismatch
Translation inhibition
Si RNA
Length 21 nt.
Cis acting
Bind with target Mrna in perfect complementary sequence
Piwi-RNA
Length ; 25 to 36 nt.
Expressed in Germ Cells
Regulates trnasposomes activity
MECHANISM OF RNAI:
First the double-stranded RNA teams up with a protein complex named Dicer, which cuts the long RNA into short pieces.
Then another protein complex called RISC (RNA-induced silencing complex) discards one of the two RNA strands.
The RISC-docked, single-stranded RNA then pairs with the homologous mRNA and destroys it.
THE RISC COMPLEX:
RISC is large(>500kD) RNA multi- protein Binding complex which triggers MRNA degradation in response to MRNA
Unwinding of double stranded Si RNA by ATP independent Helicase
Active component of RISC is Ago proteins( ENDONUCLEASE) which cleave target MRNA.
DICER: endonuclease (RNase Family III)
Argonaute: Central Component of the RNA-Induced Silencing Complex (RISC)
One strand of the dsRNA produced by Dicer is retained in the RISC complex in association with Argonaute
ARGONAUTE PROTEIN :
1.PAZ(PIWI/Argonaute/ Zwille)- Recognition of target MRNA
2.PIWI (p-element induced wimpy Testis)- breaks Phosphodiester bond of mRNA.)RNAse H activity.
MiRNA:
The Double-stranded RNAs are naturally produced in eukaryotic cells during development, and they have a key role in regulating gene expression .
2. Photosynthesis Overview
Energy for all life on Earth ultimately comes from
photosynthesis.
6CO2 + 12H2O C6H12O6 + 6H2O + 6O2
Oxygenic photosynthesis is carried out by:
cyanobacteria, 7 groups of algae,
all land plants
2
3. Photosynthesis Overview
Photosynthesis is divided into:
light-dependent reactions
-capture energy from sunlight
-make ATP and reduce NADP+
to NADPH
carbon fixation reactions
-use ATP and NADPH to synthesize organic
molecules from CO2
3
7. Discovery of Photosynthesis
The work of many scientists led to the discovery of how
photosynthesis works.
Jan Baptista van Helmont (1580-1644)
Joseph Priestly (1733-1804)
Jan Ingen-Housz (1730-1799)
F. F. Blackman (1866-1947)
7
8. Discovery of PhotosynthesisC. B. van Niel, 1930’s
-proposed a general formula:
CO2+H2A + light energy CH2O + H2O + 2A
where H2A is the electron donor
-van Niel identified water as the source of the O2 released
from photosynthesis
-Robin Hill confirmed van Niel’s proposal that energy
from the light reactions fuels carbon fixation
8
9. Pigments
photon: a particle of light
-acts as a discrete bundle of energy
-energy content of a photon is inversely proportional
to the wavelength of the light
photoelectric effect: removal of an electron from a
molecule by light
-occurs when photons transfer energy to electrons
9
11. Pigments
Pigments: molecules that absorb visible light
Each pigment has a characteristic absorption
spectrum, the range and efficiency of photons it is
capable of absorbing.
11
13. Pigments
chlorophyll a – primary pigment in plants and
cyanobacteria
-absorbs violet-blue and red light
chlorophyll b – secondary pigment absorbing light
wavelengths that chlorophyll a does not absorb
13
16. Pigments
accessory pigments: secondary pigments absorbing
light wavelengths other than those absorbed by
chlorophyll a
-increase the range of light wavelengths that can be
used in photosynthesis
-include: chlorophyll b, carotenoids, phycobiloproteins
-carotenoids also act as antioxidants
16
17. Photosystem Organization
A photosystem consists of
1. an antenna complex of hundreds of accessory
pigment molecules
2. a reaction center of one or more chlorophyll a
molecules
Energy of electrons is transferred through the antenna
complex to the reaction center.
17
20. Light-Dependent Reactions
In sulfur bacteria, only one photosystem is used for
cyclic photophosphorylation
1. an electron joins a proton to produce hydrogen
2. an electron is recycled to chlorophyll
-this process drives the chemiosmotic synthesis of
ATP
20
22. Light-Dependent ReactionsIn chloroplasts, two linked photosystems are used in
noncyclic photophosphorylation
1. photosystem I
-reaction center pigment (P700) with a peak absorption at
700nm
2. photosystem II
-reaction center pigment (P680) has a peak absorption at
680nm
22
23. Light-Dependent Reactions
Photosystem II acts first:
-accessory pigments shuttle energy to the P680 reaction
center
-excited electrons from P680 are transferred to b6-f
complex
-electron lost from P680 is replaced by an electron
released from the splitting of water
23
24. Light-Dependent Reactions
The b6-f complex is a series of electron carriers.
-electron carrier molecules are embedded in the
thylakoid membrane
-protons are pumped into the thylakoid space to form a
proton gradient
24
25. Light-Dependent Reactions
Photosystem I
-receives energy from an antenna complex
-energy is shuttled to P700 reaction center
-excited electron is transferred to a membrane-bound
electron carrier
-electrons are used to reduce NADP+
to NADPH
-electrons lost from P700 are replaced from the b6-f
complex
25
26. Light-Dependent Reactions
ATP is produced via chemiosmosis.
- ATP synthase is embedded in the thylakoid
membrane
-protons have accumulated in the thylakoid space
-protons move into the stroma only through ATP
synthase
-ATP is produced from ADP + Pi
26
28. Carbon Fixation Reactions
To build carbohydrates, cells need:
1. energy
-ATP from light-dependent reactions
2. reduction potential
-NADPH from photosystem I
28
29. Carbon Fixation Reactions
Calvin cycle
-biochemical pathway that allows for carbon fixation
-occurs in the stroma
-uses ATP and NADPH as energy sources
-incorporates CO2into organic molecules
29
30. Carbon Fixation Reactions
carbon fixation – the incorporation of CO2 into organic
molecules
-occurs in the first step of the Calvin cycle
ribulose-bis-phosphate + CO2 2(PGA)
5 carbons 1 carbon 3 carbons
The reaction is catalyzed by rubisco.
30
32. Carbon Fixation Reactions
During the Calvin cycle, energy is needed. The energy
is supplied from:
- 18 ATP molecules
- 12 NADPH molecules
32
33. Carbon Fixation Reactions
The energy cycle:
-photosynthesis uses the products of respiration as
starting substrates
-respiration uses the products of photosynthesis as
starting substrates
33