NGTS-1b is a confirmed hot Jupiter-sized extrasolar planet orbiting NGTS-1, a red dwarf star about half the mass and radius of the Sun, every 2.65 days. The NGTS-1 system is about 716 light-years from Earth in the Columba constellation.

The exoplanet, NGTS-1b, was discovered by the Next-Generation Transit Survey. Daniel Bayliss, of the University of Warwick, and lead author of the study describing the discovery of NGTS-1b, stated, "The discovery of NGTS-1b was a complete surprise to us—such massive planets were not thought to exist around such small stars—importantly, our challenge now is to find out how common these types of planets are in the Galaxy, and with the new Next-Generation Transit Survey facility we are well-placed to do just that."

NGTS-1b is a hot Jupiter-sized gas giant exoplanet that has a mass of 0.812 M_J and a radius of 1.33 R_J, where M_J and R_J are the mass and radius of Jupiter.

The planet orbits an M0.5 dwarf star about half the mass (0.617 M_☉) and radius (0.573 R_☉) of the Sun.

NGTS-1b orbits about 4.5 million km (2.8 million mi) from the host star every 2.6473 Earth-days.