NGTS-1b
Discovery | |
---|---|
Discovered by | Next-Generation Transit Survey[1] |
Discovery date | 2017 |
NGTS telescopes together with EulerCam photometric and HARPS spectroscopy followups. | |
Orbital characteristics | |
0.0326 AU (4,880,000 km)[2] | |
Eccentricity | 0.016[2] |
2.6473 JD[2] d | |
Inclination | 82.8[2] |
Star | NGTS-1[3] |
Physical characteristics | |
1.33[2] RJ | |
Mass | 0.812[2] MJ |
Temperature | 790.0[2] K |
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.[4] The NGTS-1 system is about 600 light-years from Earth in the Columba constellation.[3][1][5]
Discovery
The exoplanet, NGTS-1b, was discovered by the Next-Generation Transit Survey.[1] 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."[5]
Characteristics
Mass, radius and temperature
NGTS-1b is a hot Jupiter-sized gas giant exoplanet that has a mass of 0.812 MJ and a radius of 1.33 RJ, where MJ and RJ are the mass and radius of Jupiter.[3][1]
Host star
The planet orbits an M0.5 dwarf star about half the mass (0.617 M☉) and radius (0.573 R☉) of the Sun.[1][2]
Orbit
NGTS-1b orbits about 4.5 million km (2.8 million mi) from the host star every 2.6473 Earth-days.[3][1][2][6]
See also
References
- ^ a b c d e f Lewin, Sarah (31 October 2017). "Monster Planet, Tiny Star: Record-Breaking Duo Puzzles Astronomers". Space.com. Retrieved 1 November 2017.
- ^ a b c d e f g h i Staff (2017). "Planet NGTS-1 b". Extrasolar Planets Encyclopaedia. Retrieved 1 November 2017.
- ^ a b c d Bayliss, Danile; et al. (31 October 2017). "NGTS-1b: A hot Jupiter transiting an M-dwarf". Monthly Notices of the Royal Astronomical Society. 475 (4): 4467–4475. arXiv:1710.11099. Bibcode:2018MNRAS.475.4467B. doi:10.1093/mnras/stx2778. S2CID 39357327.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Griffini, Andrew (2 November 2017). "Huge 'monster' planet could challenge scientists' theory of how worlds form". The Times of India. Retrieved 2 November 2017.
- ^ a b Staff (31 October 2017). "'Monster' planet discovery challenges formation theory". Phys.org. Retrieved 1 November 2017.
- ^ Dvorsky, George (31 October 2017). "This Tiny Star Hosts a Planet Nearly the Size of Jupiter". Gizmodo. Retrieved 1 November 2017.
External links
- The Next Generation Transit Survey Becomes Operational at Paranal, ESO archive, The Messenger 165 – September 2016