20
C 3 Photosynthesis Chapter 10

C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Embed Size (px)

Citation preview

Page 1: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

C3 Photosynthesis

Chapter 10

Page 2: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

What you need to know!

• How photosystems convert solar energy to chemical energy.

• How linear electron flow in the light reactions results in the formation of ATP, NADPH, and O2.

• How chemiosmosis generates ATP in the light reactions.

• How the Calvin cycle uses the energy molecules of the light reactions to produce G3P

Page 3: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Photosynthesis

• Radiation energy is transformed into chemical bond energy in two distinct stages:

1. Light reactions• Occur in the thylakoid membrane• Water donates electrons to NADP+ to make

NADPH

• Water is split, O2 is released

• Photophosphorylation turns ADP into ATP

2. Calvin cycle• Occurs in the stroma

• CO2 transformed into sugar

Net Rx: 6 CO2 + 6 H2O + Light C6H12O6 + 6O2

Page 4: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Big Picture

Page 5: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Light Reactions• Location: thylakoid membrane

• Needs: Light, H2O, NADP+, ADP, P

• Makes: NADPH, O2, ATP

• Includes: Linear (non-cyclical), cyclical, & chemiosmosis

Page 6: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Linear (Non-cyclical) Light Rxs

• Photosystem II (P680) pigments absorb light (photons)

• A photon excites chlorophyll which kicks an electron e- out of the reaction center

• The excited e- is captured by the Electron Transport Chain (ETC) between P680 and Photosystem I (P700)

• The missing e- is replaced by splitting water (photolysis of water):

H2O O + 2e- + 2H+

Page 7: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Linear Light Rxs

• The excited e- moves down the ETC • The e-’s energy (excited) is used to pump H+

into the thylakoid space (creating a concentration gradient)

• e- is deposited into P700• P700 pigments absorb light (photons)• A photon excites chlorophyll which kicks an

electron e- out of the reaction center• The e- is captured by another shorter ETC• At the end of the 2nd ETC the e- binds to

NADP+• 2 e- and NADP+ are combined with H+ to form

NADPH

Page 8: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Linear Light Reactions

Page 9: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Cyclical Light Reactions

• Some e-’s, when kicked out of P700 do not go down the 2nd shorter ETC

• Instead they fall back on the first ETC between P680 and P700

• This produces less NADPH and more H+ gradient

Page 10: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Cyclical Light Reactions

Page 11: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Chemiosmosis

• This process makes ATP by using the H+ concentration gradient

• H+ concentration gradient across the thylakoid membrane means: H+ inside the thylakoid is high, while H+ in the stroma is low– On a sunny day it is 1000x’s more acidic in the

thylakoid space (pH 5 in thylakoid, pH 8 in stroma)

• ATP Synthase in the membrane functions like a turbine: when H+s rush through ATP Synthase (down the electrochemical gradient) ATP Synthase turns and uses kinetic energy to phosphorylize ADP

ADP + P ATPaka: Photophophorylation

Page 12: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light
Page 13: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Calvin Cycle

aka: light independent reactions• Location: stroma

• Needs: CO2, ATP, NADPH

• Makes: G3P, ADP, P, NADP+

Page 14: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Calvin Cycle

• Multiple enzyme pathways that uses ATP and NADPH to reduce CO2 into C6H12O6 (glucose)

• One turn of the cycle reduces one CO2

• 3 distinct steps:

1. Carbon fixation

2. Reduction

3. Regeneration

Page 15: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Carbon Fixation

• First enzyme of the cycle is Rubisco (Ribulose Bisphosphate Carboxylase) which binds 3 CO2 to an acceptor molecule RuBP

• Rubisco is the most famous and abundant enzyme on earth: no other organic molecule can chemically binding CO2

Page 16: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Reduction

• Several enzymes later the 3 CO2 have been reduced to a C3 sugar called G3P (glyceraldehyde phosphate)– powered by 6 ATP and 6 NADPH

• G3P leaves the cycle– 2 G3P can combine to form glucose

Page 17: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Regeneration

• RuBP needs to be regenerated– powered by 3 ATP

Page 18: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

3. Regeneration

1. Carbon Fixation

2. Reduction

Page 19: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Water Balance

• If water is running low, plants will close their stomata to avoid transpiration

When stomata are closed• CO2 is not replenished• ADP and NADP+ are not replenished by

the Calvin Cycle• Light Reactions run out of ADP and NADP+• Energized e-’s fall back to the reaction

center of chlorophyll– This can emit light (plant fluorescence)

Page 20: C 3 Photosynthesis Chapter 10. What you need to know! How photosystems convert solar energy to chemical energy. How linear electron flow in the light

Review

• Biology Crash Course• http://www.youtube.com/watch?v=wEPUfJ

n0s-M• Mr. Anderson (Bozeman)• http://www.youtube.com/watch?v=g78utcL

QrJ4