To obtain a copy of this paper for your own personal use please email to [email protected]. Limitations to Photosynthesis Responsible for Differences Among Speciesl J. D. Hesketh 2 AMONG species, the CO 2 assimilation varies many-fold £l. in bright sunlight. In a previous paper, photosynthesis at 1.0 Iy min. -1 (langley or cal.cm. - 2 per minute) and 300 ppm CO 2 was shown to vary from 7 to 49 mg. CO 2 dm. -2hr. --1. Further, the photosynthesis of the species with the more rapid rates continued to rise as radiation density increased above 1.0 Iy min. - 1 (3). In this report, several possible causes for these important differences among spe cies are investigated. Theoretical causes are analyzed by Rabinowitch (7). His equations predict that the maximum photosynthesis .may be determined by chlorophyll content or the propor tionality between absorbed t}uanta and photosynthesis. This . theory showed that any differences in these would be re flected in the response to dim light. Therefore, the response to low light intensities by species that vary widely in Pmax was examined. Chlorophyll concentrations were also deter mined. Alternatively, the equations predict that Pl l" " may be determined by factors in the "dark reactions," such as the quantity or renewal of the acceptor for CO 2 or by the dif . fusion of CO 2 to the site of synthesis. The theory also .... that any differences in these would be reflected in e to CO, when the CO" concentration is low. There this response as well as some of the factors affecting absorption were examined. MATERIALS AND METHODS photosynthesis of plants was measured in transparent, water·,:ooled chambers under artificial lights. The concentration of air entering and leaving the chambers was measured of an infrared gas analyzer. Air flow was measured with A fan was placed in the chamber to insure adequate un:ma(!(Jn. Details of this system for measuring photosynthesis already been presented (3). Thermocouples were fastened to bottom of the leaves by means of transparent tape. Castor bean, RichlUS commlmis L.; '.Mammoth Russian' sun Heliamhus allJIUUS L.; Conn. 870 maize, Zea mays L.; nU',,-lll!;"<"", Dt/elylis glomera/a L.; red dover, TI'ifolium pl'alellSe 'Havana Seed' tobacco, Nicotialla tabawtn L. were grown pots outdoors in May-June. In addition, some maize was grown the greenhouse. The sun-grown leaves of maple, AceI' sacchamtn and red oak, Quercus mbra L., were excised under water large trees in early June. The plants were in the vegetative of growth. The maple, maize, oak, orchardgrass, and red were growing vigorously; the castor bean, Russian sun flower, and tobacco were less vigorous than field grown plants. An attempt was made to obtain leaves capable of the maximum rate possible for the species. Leaves excised for the tree speCies as leaves for potted seedlings low photosynthetic air-free water in rates. T eave' of maize have been the field without any change in photosynthetic rates of 50 to 60 1 1'1'(. CO" d'11.""'hr.- before and after excision (unpublished data). For the photosynthetic studies between 0 and 1000 ppm CO" plants were grown in the greenhouse in the fall. To study response to light the leaves were exposed to 300 ppm CO, and temperature was maintained within a range of 2° C. while radiation was changed from 0 to 1.2 Iy min.-I. When radia tion was increased to 2.0 ly min.-i. the temperature rose 4° C. To study response to the leaves were exposed to 2.0 and 2..1 Iv min.-" except 1.2 Iy -1 was used on maple anel oak because . photosynthesis did not increase in brighter light. The great differences among these species in photosynthesis in bright light are illustrated in Figure 1. This figure exemplifies 34 curves. At 1 Iy min.-' the photosynthesis of maize was eight fold that of maple. Further, the rate of maize was still rising with increasing I1ght while that of maple was constant at all light inten sities above 0.25 ly min.->' The response of sunflower resembles that of maize; tobacco, red dover, and castor bean resemble that of orchard grass. These can all be seen in the first 2 columns of data in Table 1 where 34 observations are summarized by ranges of Thus these species provide a wide range in P a,.,: in which causes variation might be discovered. RESULTS Response to Light As stated earlier, Pm.." may be determined by chlorophyll content or the proportionality between photosynthesis and absorbed quanta. These factors also determine the slope of the light response curve at low radiation density I. The rectangular hyperbola Q _ Qm.."KI (1 + KI)-l [1] has satisfactorily fit Q, (net photosynthesis plus respiration in the dark), when related to a wide range of 1. Q"H'X is Q as I -;... 00. QmaxK is the slope of the response curve as 1-+0. Qm..x K is, therefore, the critical characteristic. Unfortu nately its variation is poorly revealed near the crowded origin of graphs such as Figure 1. If, however, we trans form equation [1] into IJQ - IJQm.." + I/Qm..J< K [2] Qm." K becomes the intercept, Figure 2. Where I > 0.25, equation [2] fits the data well. Where I < 0.25, the four sets of data in Figure 2 (as well as the 30 additional ones not shown in the figure) all require a curvilinear relation rather than equation [2]. As light de creases to 0.25 ly min. respiration becomes at least one fifth of Q. The departure from equation [2] where I < 0.25 may, therefore, be caused by the questionable estima tion of photosynthesis as net photosynthesis plus respira tion in the dark where the latter is relatively large. Where I > 0.25, equation [2] does, nevertheless, fit the data well. Extrapolation to I - 0 of the lines through these data indicates that the lines all intersect the ordinate 60 ' 50 Maize ..c 't E 40 '0 0'30 o Ol - E 20 I 1 Investigations supported by Natioml Science Foundation and C0 .flflecticllt funds. Received Jan. 31, 1963. - Formerly Assistant Crop Physiologist, The Connecticut tuml Experiment Station. New Haven. now Assistant Plant University of Arizona, Tucson. Uy min-I) Figure I-Relation to light intensity I of the photosynthesis Q of 4 species. The 2.0 Iy min.-1 is equivalent in quanta to 10,000 ft.-c. of sunlight. 493
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