Abstract
As a thermogenic organ, heat generation and loss within and from the mammalian brain may play a role in determining its shape. We investigated brain shape by comparing endocranial volume (EcV, a proxy of heat generating tissue) and endocranial surface area (EcSA, a proxy of convective heat loss) in 472 species using phylogenetically appropriate methods. A distinct ancestral mammalian condition in the relationship between EcV and EcSA was found. Rodentia exhibit a more tubular brain shape, while Cercopithecoidea, Hominoidea, and Neoceti show a more spherical brain. Increased brain sphericity will reduce heat loss, providing energetic savings important in the context of natural selection.
| Original language | English |
|---|---|
| Title of host publication | Evolution of Nervous Systems |
| Editors | Jon H. Kaas, Suzana Herculano-Houzel |
| Publisher | Elsevier |
| Chapter | 2.01 |
| Pages | 1-40 |
| Number of pages | 40 |
| Volume | 2 |
| Edition | 3rd |
| ISBN (Electronic) | 9780443273810 |
| ISBN (Print) | 9780443273803 |
| DOIs | |
| Publication status | Published - 2026 |
Keywords
- Brain
- Evolution
- Heat loss
- Heat production
- Hominoidea
- Neoceti
- Rodentia
- Thermodynamics
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