Tokenized Real-World Assets (RWAs) are expanding into bonds, treasuries and other traditional assets being brought on-chain. And now, the use case is the real concern. Tokenised RWAs hit $30B! Tokenized RWAs have crossed the $30 billion-mark, with the market very quickly expanding since 2025. This category was once mainly associated with stablecoins. Today, it's spreading across treasuries, private credit, commodities, equities, funds, and other yield-bearing assets. It's not just that traditional assets are moving on-chain. It is that they can now become part of real activity. Capital can be put to work, collateral can become more usable, and yield can connect with credit and trading! What's causing the growth? According to CoinGecko, tokenized RWAs have more than tripled since the start of 2025. In fact, by the end of Q1 2026, it had climbed to $19.3B. Even though the sector is still much smaller than stablecoins, its growth has been faster over the past year. As for the asset mix? Bonds dominate the on-chain RWA market at 60.2%, or around $16B. Precious metals come next at 21.6%, followed by private credit at 9.9%. Together, just these three categories make up 92% of the market. RWAs need to become usable, not just tokenized This concentration is not a weakness by itself. In fact, it shows where early demand is strongest. These are assets that already have clear value, yield, or collateral use cases. But the growth will not come from just putting more assets on-chain. RWAs need better integration into the rest of crypto markets. Tokenized bonds, metals, and credit products should be easier to use as yield-bearing positions. Otherwise, they risk becoming on-chain wrappers that people hold, but don't use. The real unlock is utility! Final Summary Tokenized RWAs have crossed $30 billion, with bonds alone accounting for over 60% of the market. The next phase of RWA growth depends on making assets usable across strategies and collateral markets.
The $30B RWA boom has arrived, but the real challenge is just beginning!
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