Enteric Fermentation: origin of gases, variations, predictions and - - PowerPoint PPT Presentation

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Enteric Fermentation: origin of gases, variations, predictions and - - PowerPoint PPT Presentation

Enteric Fermentation: origin of gases, variations, predictions and mitigation Michael Blmmel Outline of Presentation Origin of ruminal CO 2 and CH 4 from fermentation products Causes and implications of variations in ruminal CO 2 and CH


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Enteric Fermentation: origin of gases, variations, predictions and mitigation

Michael Blümmel

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Outline of Presentation

Origin of ruminal CO2 and CH4 from fermentation products Causes and implications of variations in ruminal CO2 and CH4 Stochiometry of CO2 and CH4 production Prediction of CO2 and CH4 production in vitro and in vitro Enteric mitigation options

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OMTDR SCFA MBP GAS

= + +

MBP SCFA GAS Short chain fatty acids (C2, C3, C4) supply energy to host animal Microbial biomass supplies protein to host animal ( but also CHO, lipids) CH4 und CO2 ,losses to rumen Microbes and host animal alike

  • Principles Generalization of ruminal

microbial feed degradation

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HEXOSE SCFA

C-C-C-C-C-C

2 Acetate (2 X C-C)

C-C-C-C-C-C

2 Propionate (2 X C-C-C)

C-C-C-C-C-C

1 Butyrate (1 X C-C-C-C)

Carbon Utilization from Hexose in Microbial Short-Chain Fatty Acid (SCFA) Production

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Stoichiometrical calculation of CO2 and

CH4 from SCFA ratio (C2:C3:C4) according to Wolin (1960)

Principle: balance of net oxidation values is zero Example 1 mol of SCFA with 0.65a; 0.25p; 0.1b CO2 = a/2 + p/4 + 1.5 * b CO2 = 0.65/2 + 0.25/4 + 1.5 * 0.1 CO2 = 0.54

(see Van Soest, 1994, pp 272 – 275)

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Generally, CH4 is produced from CO2

CO2 + 8H > CH4 + 2* H20 Stoichiometrically (Wolin, 1960) CH4 = a + 2*B - CO2 CH4 = 0.65 + 0.2 – 0.54 CH4 = 0.31

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15 25 35 45 55 65 75 85 95 105 115 125 15 25 35 45 55 65 75 85 95 105 115 125

Diets and compound feeds N = 38 Components N = 27 Forages and roughages N = 57

y= -3.1 + 1.03x; R

2

= 0.96 Sy.x = 4.2; P < 0.0001

SBM

24 h gas volumes (ml) stoichiometrically calculated 24 h measured gas volumes (ml) after pressure correction

Comparisons of stoichiometrically calculated and observed in vitro gas volumes

(Blümmel et al 1999)

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Stochiometry

Powerful, simple and inexpensive tool to predict gases from SCFA amount and proportion Generally good agreement between lab / in vitro and in vivo data More complex with substrates/feeds high in protein and anti-nutritive factors Limited application to hindgut fermentation

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Variations in ratios of products of ruminal microbial feed degradation

High Efficiency of Microbial Production (EMP) Low Efficiency of Microbial Production (EMP)

OMTDR OMTDR SCFA MBP GAS

= + +

SCFA MBP GAS

+ + =

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Many feeding systems treat microbial production as a constant, despite acknowledged variation in EMP Lack of simple techniques to detect and predict variations in EMP

Mean EMP Range in EMP Stern & Hoover (1979) 30 g MN /OMTDR 10 – 50 g MN / OMTDR Lebzien (1996) 10.3 g MP / MJ MEI 7.1 – 14.0 g MP / MJ MEI

EMP in vivo: data from literature review

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11

Pansen 10 kg Futter mikrobiell abgebaut

8 kg DM intake

Relevance of EMP for Carbon Emissions

Assumptions: EMP Diet 1 = 0.10 and EMP Diet 2 = 0.40 Digestibility 63%

5 kg degraded in the rumen

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CO2 : 513 l (1008 g) CH4 : 296 l (211 g) 4.5 kg: C2, C3, C4, CO2, CH4 0.5 kg: Microbial biomass 3.0 kg:C2, C3, C4, CO2, CH4 2.0 kg: Microbial biomass CO2: 324 l (673 g) CH4: 197 l (140 g)

Urine-N

Diet 2 (8 kg) Diet 1 (8 kg)

Urine-N

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Efficiency of microbial production

Variations in EMP are real and have significant effects on variations in enteric GHG emissions Maximizing EMP regardless of specific P: E host animal requirement Not applicable to hindgut fermentation How to detect variations in EMP?

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OMTDR SCFA MBP GAS

= + +

Approaches: detecting variations in EMP

Possible measurements:

  • 1. All three degradation products
  • 2. Two products and OMTDR like:

MBP = OMTDR – [SCFA + GAS]

  • 3. One product and OMTDR if firm

linkage exists between this and one

  • ther product
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Exemplary: One mmol of SCFA in proportion

0.65a: 0.25p: 0.10b results in 1. 0.54 mmol CO2 (23.4 mg) 2. 0.31 mmol CH4 ( 5.0 mg) 3. 0.65 mmol a (39.0 mg) 4. 0.25 mmol p (18.5 mg) 5. 0.10 mmol b ( 8.8 mg)

  • 6. 2x0.35 mmol H2O

(11.2 mg) 105.9 mg Gas volume: 0.54 mmol CO2 13.8 ml 0.31 mmol CH4

7.9 ml

1.00 mmol CO2BUFF 25.6 ml 47.3 ml SF = 105.9 mg: 47.3 ml = 2.24 mg/ml

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Accepting a stoichiometric factor (SF)

  • f 2.2 mg H, C, O for 1 ml of gas,

MBP can be calculated as:

MBP = OMTDR – [GAS * 2.2] Requirements:

  • 1. Gas volume
  • 2. OMTDR

Observe: SF at high propionate (>40%) equals 2.34 mg/ml

(Blmmel et al. 1997

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500 mg substrate supplied 325 mg feed degraded as determined by ND- solution treatment (Goering and Van Soest (1970) 130.6 ml gas 87.5 ml gas

EMP 0.1 EMP 0.4

EMP = (325 – [130.6 * 2.2])/325 EMP = 0.12

EMP = (325 – [87.5 * 2.2])/325 EMP = 0.41

Predicting in EMP in vitro by gas volumes, OMTDR and SF

175 mg 175 mg

(Blummel et al 1997)

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500 mg substrate supplied 325 mg feed degraded as determined by ND- solution treatment (Goering and Van Soest (1970) 130.6 ml gas 87.5 ml gas

EMP 0.1 EMP 0.4

PF = 325 mg/130.6 ml PF = 2.49 mg/ml PF = 325 mg /87.5 ml PF = 3.74 mg/ml

Partitioning Factor: high degradability but proportionally low gas production

175 mg 175 mg

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500 mg substrate 90.8 ml gas 68.5 ml gas

Residue 235.8 mg Residue 236.0 mg Wheat Straw Trifol. Wheat Straw

Partitioning Factor: actually measured after 24-h of incubation

PF = 264.2 mg / 90.8 ml PF = 2.91 mg/ml PF = 264.0 mg / 68.5 ml PF = 3.85 mg/ml

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Comparison of predicted and measured CH

4

production

10 15 20 25 30 35 40 10 15 20 25 30 35 40 NaOH treated straws Untreated straws NH

4

treated straws y=3.8 + 0.82x; R

2 = 0.88; P<0.0001; Sy.x=2.5

CH

4

(l) predicted based on in vitro variables and voluntary feed intake CH

4

(l) measured in respiration chambers

(Blümmel et al 2005)

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Relations between digestible organic matter intake and methane production in sheep

100 200 300 400 500 600 700 800 900 5 10 15 20 25 30 35 40 y = 5.6 + 0.037x, R

2

= 0.82, P<0.0001 HOWEVER: 35.4 to 63.7 l/kg DOMI Digestible organic matter intake in sheep (g/d) Methane production in sheep (l/d)

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Predicting GHG in vivo Major driver intake, feed quality next

With intake and diet quality known, GHG can be predicted with reasonable accuracy Intake and quality often unknowns, opportunistic, variable in small holder systems

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Mitigation of enteric GHG

  • 1. Feed manipulation (SCFA/ EMP)
  • 2. Feed allocation, intensification
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Combined SCFA and EMP effects on methane production

100 150 200 250 300 350 400 17.5 22.5 27.5 32.5 37.5 42.5 47.5 52.5 57.5 62.5 67.5 high concentrate (high propionate) high roughage (high acetate)

Microbial biomass produced per kg feed digested (g/kg) CH4 (l) produced per kg feed digested

Blümmel and Krishna 2003

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25

Across herd milk yields (3.61 kg/d) in India and scenario-dependent ME needs for total milk production (81.8 million t/y)

ME required (MJ x 109) Milk (kg/d) Maintenance Production Total 3.61 (05/06) 1247.6 573.9 1821.5 6 (Scenario 1) 749.9 573.9 1323.8 9 (Scenario 2) 499.9 573.9 1073.8 12 (Scenario 3) 374.9 573.9 948.8 15 (Scenario 4) 299.9 573.9 873.9

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26

Effect of increasing average daily milk yields on

  • verall methane emissions from dairy in India

3 6 9 12 15 0.0 0.5 1.0 1.5 2.0 2.5 Daily milk yield per animal (liter)

Methane produced (Tg)

current herd average milk yield of 3.61 l/d (Blmmel et al. 2009)

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Mitigation of enteric GHG

1. Feed manipulation (SCFA/ EMP)

Biologically feasible, however, multiple trade-offs involved, economically largely untested, difficult to apply to small holder systems

  • 2. Feed allocation, intensification

Feasible and bound to happen. However, important non-technical support required such as credit, insurance, labor issues etc

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Thank you for your attention

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Efficiency of Microbial Production

SCFA Gases MBP EMP = 0.1 EMP = 0.4 1 kg OMTDR SCFA : 562 g 375 g 225 g MBP: 400 g

LEGENDS

  • SCFA: 0.65 a: 0.25 p : 0.10 b

(Blmmel et al. 2001)

Gases: 338g 100 g

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Efficiency of Microbial Production

SCFA Gases MBP EMP = 0.1 EMP = 0.4 1 kg OMTDR SCFA : 611 g 407g 193 g MBP: 400 g

LEGENDS

  • SCFA: 0.50 a: 0.40 p : 0.10 b

Gases:289 g 100 g

(Blmmel et al. 2001)

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EMP and host animal requirement of protein: energy Problem: If MBP > protein requirement of host

MBP used for energy EMP 0.4 – 0.1 300 g MBP 3.3 MJ from SCFA 2.94 MJ NE (f) 1.94 MJ NE (f) HOWEVER ↑

↑ ↑ ↑ RENAL N EXCRETION

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Predicting GHG in vivo Major driver intake, feed quality next

With intake and diet quality known, GHG can be predicted with reasonable accuracy Intake and quality often unknowns, opportunistic, variable in small holder systems

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2 4 6 8 10 12 14 16 18 20 22 24

17 18 19 20 21 22 23 24 25 D I (0.778) D II (0.788) D III (0.817) D IV (0.780) D V (0.830)

25 g N: kg OM LEGENDS Release of N: OM during 24 hrs Ratio N: OM

Release of N and OM during 24 hrs incubation in five iso-nitrogenous diets

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0.76 0.77 0.78 0.79 0.80 0.81 0.82 0.83 0.84 0.85 0.86 30 31 32 33 34 35 36 37 38 y = - 29.3 + 78.8 x; R

2

= 0.89; P = 0.02 Synchronization Index Efficiency of microbial production ( g MBP/100 g OMTDR) in sheep)

Relationship between synchronization Indices and EMP in sheep