# Collapsar

> As of Nov 5, 2026, Collapsar has no recorded sale.

- Page: https://www.gondi.xyz/collections/makersplace-2963/16533
- Collection: [MakersPlace](https://www.gondi.xyz/collections/makersplace-2963.md)
- Token ID: [16533](https://etherscan.io/nft/0x2963ba471e265e5f51cafafca78310fe87f8e6d1/16533)
- Contract: [0x2963ba471e265e5f51cafafca78310fe87f8e6d1](https://etherscan.io/address/0x2963ba471e265e5f51cafafca78310fe87f8e6d1) (ERC-721)
- Owner: [Gydra](https://www.gondi.xyz/0xe9f1c3cf268e67d2bad6c410156afc2d063ad4e7)
- Image: https://i2c.seadn.io/ethereum/0x2963ba471e265e5f51cafafca78310fe87f8e6d1/2073940d705ff902fa002510a2e1f7/c52073940d705ff902fa002510a2e1f7.jpeg?w=1000

## Description

A collapsar is a star which has undergone gravitational collapse. When a star no longer has enough fuel for significant fusion reactions, there are three possible outcomes, depending on the star's mass: If it is less than the Chandrasekhar limit (1.4 solar masses), the star will stabilize and shrink, becoming a white dwarf; between the Chandrasekhar limit and the Tolman–Oppenheimer–Volkoff limit (approximately 3 solar masses), it will become a neutron star; and above the Tolman–Oppenheimer–Volkoff limit, the star will become a black hole. However, it is theorized that the high density of neutron star cores allow for quark matter and, as a result, a star that is more massive than even the Tolman–Oppenheimer–Volkoff limit, yet still isn't a black hole.

Data from GONDI (https://www.gondi.xyz), Nov 5, 2026.