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Do different star types produce plants with different properties?

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From this chart it appears that the star types closest to our own are K-type (oranger, a little cooler, and less than half as bright) and F-type (bluer, a little warmer, and much brighter). If I want to place an "earth-like" planet around one of these star types, how should I expect plant life on my planet to develop differently compared to Earth?

By "earth-like" I mean a planet that has temperature, terrain, water, and atmosphere conducive to the development of higher life forms (eventually sentient ones). How does the star type affect the appearance, growth, types, density, etc of plants? Should one star type lead to denser (or sparser) jungles, taller (or shorter) trees, different kinds of fruits, etc?

I think this question is related. I don't know enough chemistry to say how related, though.

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Let's think about this in terms of peak emission. Wien's displacement law tells us that the peak emission wavelength of a black body, λmax, is inversely proportional to its temperature, T: λmax=bT where b is Wien's displacement constant; b2.9×103 m K. Using this and some assumptions about temperature, we can determine the peak of a star's spectrum, given that most stars are well-approximated as black bodies. Here, we assume that T is the star's effective temperature, and pick a temperature in the general range of each type. I'm going to use the Harvard spectral classification. Star typeColorT(K)λmax(nm)Oblue35,00082.9Bblue-white20,000145Awhite8,000363Fyellow-white7,000414Gyellow5,500527Korange4,000725Mred3,000967 Next, we have to assume that the plants are somewhat like the ones found on Earth - they use the same compounds and processes to survive. Life on Earth is all that currently exists in our dataset, and it's all we have to work with before delving into too much speculation.

One important process is photosynthesis. There are a variety of photosynthetic pigments available. I was able to find a book chapter detailing many of them along with their key property here, the wavelength(s) of maximum absorption λabs. Here's a table of the relevant ones: Pigmentλabs(nm)OccurrenceChlorophyll a435,670-680Photosynthetic plantsChlorophyll b480,650Higher plants; green algaeChlorophyll c435,645Diatoms; brown algaeChlorophyll d435,740Red algaeChlorobium chlorophyll750,760Green bacteriaBacteriochlorophyll a800,850,890Purple bacteria; green bacteriaBacteriochlorophyll b435,740Rhodopseudomonas (a purple bacterium)α-Carotene420,440,470Leaves; red algae; green algaeβ-Carotene425,450,480Most other plantsγ-Carotene440,460,495Green sulfur bacteriaLuteol425,445,475Green leaves; green algae; red algaeViolaxanthol425,450,475LeavesFucoxanthal425,450,475Diatoms; brown algaeSpirilloxanthal464,490,524Purple bacteriaPhycoerythrins490,546,576Red algae; some blue-green algaePhycocyanins618Blue-green algae; some red algaeAllophycocyanin654Blue-green algae; red algae The Sun's λmax, is in the neighborhood of 500 nm, landing it smack in the middle of all these pigments - as would be expected. I have some immediate observations:

  • Many pigments have favorable absorption in the 420-500 nm range, near λmax,.
  • There are a couple other peaks, from 618-680 nm, 740-760 nm, and 800-890 nm. These are mainly due to pigments used by certain types of bacteria.

It stands to reason that if λmax, was somewhere else, different pigments would dominate. So let's add a couple columns to our first table: Star typeλmax(nm)Possible dominant pigmentsPossible dominant plantsO82.9?AlgaeB145?AlgaeA363Miscellaneous algal pigmentsGreen and brown algae; some red algaeF414ChlorophyllsHigher plants; green, brown and red algaeG527ChlorophyllsHigher plants; blue-green algaeK725BacteriochlorophyllsPurple bacteria; green bacteria; blue-green algaeM967BacteriochlorophyllsPurple bacteria; green bacteria I've stated that algae would be the most likely plants on planets orbiting O- and B- type stars. This has nothing to do with pigments; rather, it is because these stars are so short-lived that multicellular life would have a hard time developing there. In fact, age may impact the types of life you would see across the board. More massive stars have less time for higher life to develop and so probably won't lead to complicated, multicellular life.

I still have to agree, at least in part, with Ville Niemi's answer. It's clear that plenty of different pigments exist on Earth, and there's no reason to think we wouldn't see even others on an alien world around a different star. However, in drastic enough cases (especially with M-dwarfs and O and B stars), there likely would be major shifts in the dominant pigments. Perhaps new ones would develop, and I can't speculate on those. I can, though, tell you which ones would gain some slight advantages. So maybe view this answer as saying "Well, maybe [X, Y, Z]" rather than something definitive, especially given that I'm no expert.

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