Observations of Planet Formation Around the Protostar HOPS-315 and Implications for the Formation of the Solar System

Author(s)	Ritika Pannu
Country	India
Abstract	We can now watch planets taking shape around other stars as it happens. With tools like ALMA and the James Webb Space Telescope, astronomers get an up-close look at young star systems. For example, HOPS-315—a protostar—has hot silicate minerals forming in its disk. They remind us of the calcium–aluminum-rich inclusions found in ancient meteorites from our own Solar System. In this paper, I line up HOPS-315’s features against the Solar Nebula model and meteorite data. The parallels—like the spinning disk and those early, high-temperature solids—make it pretty clear our Solar System likely formed through the same steps we’re now seeing unfold in new stars.
Published In	Volume 7, Issue 4, April 2026
Published On	2026-04-17
DOI	https://doi.org/10.70528/IJLRP.v7.i4.2122
Short DOI	https://doi.org/hbxntk

About IJLRP Fees & Payment Current Issue Publication Archive	Submit Research Paper Track Submission Status Publication Guidelines Publication Ethics Peer Review & Plagiarism	Join as a Reviewer Editors & Reviewers Reviewer Referral Program Get Reviewer Membership Certi.	Website/Journal Policies Usage Policy Content Policies Privacy Policy

Contact Us		+91-9687-828-838	editor@ijlrp.com

International Journal of Leading Research Publication