The Space-based multi-band Variable Objects Monitor (SVOM) mission, launched into low Earth orbit on 2024 June 22, is a French-Chinese multi-wavelength observatory dedicated to the study of the transient sky. Inspired by the Neil Gehrels Swift Observatory, it consists of an autonomous rapid-slewing satellite, linked in real time to several ground-based telescopes. The space segment comprises two X-ray/gamma-ray wide-field instruments (ECLAIRs and Gamma-Ray Monitor) with real-time triggering capabilities combined with two narrow-field telescopes in X-ray (MXT) and in the VT. In addition, the SVOM collaboration has also developed a unique visible and NIR ground-based follow-up system to promptly respond to the gamma-ray transients detected onboard. The Core Program of SVOM will provide new insights into the gamma-ray burst physics by providing a homogeneous dataset covering both the prompt and afterglow emissions, as well as better studying the low luminosity and soft gamma-ray burst populations. As a versatile satellite platform with fast slewing capabilities, SVOM also comprises a Target of Opportunity program and a General Program consisting of pointed observations scheduled over the year that will both significantly contribute to the multi-messenger and time-domain aspects of astronomy.