Loading…
Phenotypic relationships among oil, protein, fatty acid composition and seed size traits in Cucurbita pepo
•There is wide variation in oil, protein and fatty composition within C. pepo.•Seed oil and seed protein are negatively correlated.•Seed size is positively correlated with seed oil but negatively correlated with seed protein.•‘Naked’ seed accessions are higher in oil and greater in seed size than hu...
Saved in:
Published in: | Scientia horticulturae 2018-03, Vol.233, p.47-53 |
---|---|
Main Authors: | , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | •There is wide variation in oil, protein and fatty composition within C. pepo.•Seed oil and seed protein are negatively correlated.•Seed size is positively correlated with seed oil but negatively correlated with seed protein.•‘Naked’ seed accessions are higher in oil and greater in seed size than hulled accessions.
Pumpkin seed (Cucurbita pepo L.) is high in oil, protein and total unsaturated fatty acids (TUFA), and provides an important source of nutrition and income globally. Use of pumpkin seed in the snacking and vegetable oil industry in the U.S. is expected to rise as the market for healthy foods increases. Currently, most of the pumpkin seed consumed in the U.S. is imported, and there is need to breed high-yielding and nutritious cultivars that are locally adapted to various agro-ecological growing zones in the country. In the current study, phenotypic variation of key seed nutrition traits among 35C. pepo accessions of different seed phenotypes (hulled, semi-hulled, thin layer and ‘naked’) was determined with the primary goal of identifying the best parental material for breeding as well as elucidating phenotypic relationships among the traits. Seed oil percentage ranged from 29.33% to 48.41% and was significantly (P |
---|---|
ISSN: | 0304-4238 1879-1018 |
DOI: | 10.1016/j.scienta.2018.01.030 |