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The Importance of Hope with Phil Clayton (Part 1)

The Importance of Hope with Phil Clayton (Part 1)

FromHunger for Wholeness


The Importance of Hope with Phil Clayton (Part 1)

FromHunger for Wholeness

ratings:
Length:
30 minutes
Released:
Aug 15, 2022
Format:
Podcast episode

Description

In this episode Hosts, Ilia Delio and Gabby Sloan interview Author, Teacher, Activist, Phil Clayton as they discuss the following themes:“If as individuals, tribes, and cultures, we are in continual development; if our planet, and indeed our very universe, continually evolves into newness; then how can we not imagine that the Christ would also be a part of a cosmic becoming?” Phil ClaytonPhilip Clayton, Ingraham Professor at Claremont School of Theology, writes and speaks widely on the evolution of human consciousness and spirituality. Co-Director of the Center for Process Studies (ctr4process.org) and author or editor of two dozen books and some 300 articles, he advocates for an evolutionary metaphysics and ethics beyond the old “warfare” of science and theology. Increasingly, he is being drawn to the intersection of climate science, ethics, religion ― ecotheology.Support the showA huge thank you to all of you who subscribe and support our show! This podcast is made possible by a grant from the The Fetzer Institute . We are very grateful for their support. Join our our Patreon 'Hunger for Wholeness' Community for further background materials. Follow us on Facebook, Instagram and Twitter.
Released:
Aug 15, 2022
Format:
Podcast episode

Titles in the series (62)

Story matters. Our lives are shaped around immersive, powerful stories that thrive at the heart of our religious traditions, scientific inquiries, and cultural landscapes. As Bertrand Russell and Albert Einstein claimed, science without religion is lame and religion without science is blind. This podcast will hear from speakers in interdisciplinary fields of science and religion who are finding answers for how to live wholistic lives. This podcast is made possible by funding from the Fetzer Institute. We are very grateful for their generosity and support.Image credit:X-ray: NASA/CXC; Ultraviolet: NASA/JPL-Caltech/SSC; Optical: NASA/STScI(M. Meixner)/ESA/NRAO(T.A. Rector); Infrared: NASA/JPL-Caltech/K. Su