Kepler-11

Kepler-11

Artist's conception of a simultaneous transit of three planets before Kepler-11 observed by NASA's Kepler spacecraft on Aug. 26, 2010.
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 48m 27.622s[1]
Declination +41° 54′ 32.87″[1]
Apparent magnitude (V) 14.2[2]
Astrometry
Proper motion (μ) RA: –0.7[1] mas/yr
Dec.: –4.1[1] mas/yr
Distance613[2] pc
Characteristics
Spectral type G6V[3]
Details
Mass0.961+0.025
−0.025[4] M☉
Radius1.065+0.017
−0.022[4] R☉
Luminosity1.045+0.061
−0.078 L☉
Surface gravity (log g)4.366+0.014
−0.016[4] cgs
Temperature5663+55
−66[4] K
Metallicity [Fe/H]0 (± 0.1)[5] dex
Age8.5+1.1
−1.4[4] Gyr
Other designations

Kepler-11 is a Sun-like star slightly larger than the Sun in the constellation Cygnus, located some 2,000 light years from Earth.[3][6] It is located within the field of vision of the Kepler spacecraft, the satellite that NASA's Kepler Mission uses to detect planets that may be transiting their stars. Announced on February 2, 2011, the star system is among the most compact and flattest systems yet discovered. It is the first discovered case of a star system with six transiting planets. All discovered planets are larger than Earth, with the larger ones being about Neptune's size.

Nomenclature and history

Kepler-11 and its planets were discovered by NASA's Kepler Mission, a mission tasked with discovering planets in transit around their stars. The transit method that Kepler uses involves detecting dips in brightness in stars. These dips in brightness can be interpreted as planets whose orbits move in front of their stars from the perspective of Earth. Kepler-11 is the first discovered exoplanetary system with more than three transiting planets.[7]

Kepler-11 is named for the Kepler Mission: it is the 11th star with confirmed planets discovered in the Kepler field of view. The planets are named alphabetically, starting with the innermost: b, c, d, e, f, and g, distinguishers that are tagged onto the name of their home star.

The orbit of the Kepler-11 planets in comparison to orbits of planets Mercury and Venus.

Characteristics

Kepler-11 is a G-type star that is approximately 96% the mass of and 107% the radius of the Sun. It has a surface temperature of about 5663 K and is estimated to have an age of around 8.5 billion years.[4] In comparison, the Sun is about 4.6 billion years old[8] and has a surface temperature of 5778 K.[9]

The star's apparent magnitude, or how bright it appears from Earth's perspective, is 13.7. Therefore, it cannot be seen with the naked eye.[5]

Planetary system

All known planets transit the star; this means that all six planets' orbits appear to cross in front of their star as viewed from the Earth's perspective. Their inclinations relative to Earth's line of sight, or how far above or below the plane of sight they are, vary by a little more than a degree. This allows direct measurements of the planets' periods and relative diameters (compared to the host star) by monitoring each planet's transit of the star. Simulations suggest that the mean mutual inclinations of the planetary orbits are about 1°, meaning the system is probably more coplanar (flatter) than the Solar System, where the corresponding figure is 2.3°.[3]

The estimated masses of planets b - f fall in the range between those of Earth and Neptune. Their estimated densities, all lower than that of Earth, imply that none of them have an Earth-like composition;[10] a significant hydrogen/helium atmosphere is predicted for planets c, d, e, f, and g, while planet b may be surrounded by a steam atmosphere or perhaps by a hydrogen atmosphere.[11][12] The low densities likely result from high-volume extended atmospheres that surround cores of iron, rock, and possibly H2O.[12][13] The inner constituents of the Kepler-11 system were, at the time of their discoveries, the most comprehensively understood extrasolar planets smaller than Neptune.[14] Currently, observations do not place a firm constraint on the mass of planet g (<25 ME).[11] However, formation and evolution studies indicate that the mass of planet g is not much greater than about 7 ME.[12]

Kepler-11 planets may have formed in situ (i.e., at their observed orbital locations) or may have started their formation farther away from the star while migrating inward through gravitational interactions with a gaseous protoplanetary disk. This second scenario predicts that a substantial fraction of the planets' mass is in H2O.[12] Regardless of the formation scenario, the gaseous component of the planets accounts for less than about 20% of their masses but for ≈40 to ≈60% of their radii.

The system is among the most compact known; the orbits of planets b - f would easily fit inside the orbit of Mercury, with g only slightly outside it. Despite this close packing of the orbits, dynamical integrations indicate the system has the potential to be stable on a time scale of billions of years.[3]

None of the planets are in low-ratio orbital resonances, in which multiple planets gravitationally tug on and stabilize each other's orbits, resulting in simple ratios of their orbital periods.[13] However, b and c are close to a 5:4 ratio.[3]

There could conceivably be other planets in the system that do not transit the star, but they would only be detectable by the effects of their gravity on the motion of the visible planets (much as how Neptune was discovered).

Planet Mass
(ME)		 Radius
(RE)		 Density
(g/cm3)		 Orbital
period
(d)		 Semimajor
axis
(AU)		 Orbital
ecc.		 Inc.
(°)		 Discovery
year
b 1.9+1.4
−1.0 		1.8+0.03
−0.05 		1.72+1.25
−0.91 		10.3039+0.0006
−0.0010 		0.091+0.001
−0.001 		0.045+0.068
−0.042 		89.64+0.36
−0.18 		2011[4]
c 2.9+2.9
−1.6 		2.87+0.05
−0.06 		0.66+0.66
−0.35 		13.0241+0.0013
−0.0008 		0.107+0.001
−0.001 		0.026+0.063
−0.013 		89.59+0.41
−0.16 		2011[4]
d 7.3+0.8
−1.5 		3.12+0.06
−0.07 		1.28+0.14
−0.27 		22.6845+0.0009
−0.0009 		0.155+0.001
−0.001 		0.004+0.007
−0.002 		89.67+0.13
−0.16 		2011[4]
e 8.0+1.5
−2.1 		4.19+0.07
−0.09 		0.58+0.11
−0.16 		31.9996+0.0008
−0.0012 		0.195+0.002
−0.002 		0.012+0.006
−0.006 		89.89+0.02
−0.02 		2011[4]
f 2.0+0.8
−0.9 		2.49+0.04
−0.07 		0.69+0.29
−0.32 		46.6888+0.0027
−0.0032 		0.250+0.002
−0.002 		0.013+0.011
−0.009 		89.47+0.04
−0.04 		2011[4]
g <25 3.33+0.06
−0.08 		<4 118.3807+0.0010
−0.0006 		0.466+0.004
−0.004 		<0.15 89.87+0.05
−0.06 		2011[4]

Relative size and positions of the 6 planets of Kepler-11, and of the innermost Solar System for comparison.
The diameters of the planets (but not of the stars) are scaled up by a factor of 50.

See also

References

  1. 1 2 3 4 Zacharias, N.; et al. (June 2010). "The Third US Naval Observatory CCD Astrograph Catalog (UCAC3)". The Astronomical Journal. 139 (6): 2184–2199. arXiv:1003.2136Freely accessible. Bibcode:2010AJ....139.2184Z. doi:10.1088/0004-6256/139/6/2184.
  2. 1 2 3 "Kepler Discoveries". NASA Ames Research Center. Retrieved 4 February 2011.
  3. 1 2 3 4 5 Lissauer, J. J.; et al. (3 February 2011). "A closely packed system of low-mass, low-density planets transiting Kepler-11". Nature. 470 (7332): 53–58. arXiv:1102.0291Freely accessible. Bibcode:2011Natur.470...53L. doi:10.1038/nature09760. PMID 21293371.
  4. 1 2 3 4 5 6 7 8 9 10 11 12 Lissauer, Jack J.; Jontof-Hutter, Daniel; Rowe, Jason F.; Fabrycky, Daniel C.; Lopez, Eric D.; Agol, Eric; Marcy, Geoffrey W.; Deck, Katherine M.; Fischer, Debra A.; Fortney, Jonathan J.; Howell, Steve B.; Isaacson, Howard; Jenkins, Jon M.; Kolbl, Rea; Sasselov, Dimitar; Short, Donald R.; Welsh, William F. (2013). "All Six Planets Known to Orbit Kepler-11 Have Low Densities". The Astrophysical Journal. 770 (2): 131. arXiv:1303.0227Freely accessible. Bibcode:2013ApJ...770..131L. doi:10.1088/0004-637X/770/2/131.
  5. 1 2 "Planet Kepler-11 b". The Extrasolar Planet Encyclopedia. Retrieved 4 July 2014.
  6. ↑ Astronomers Find 6-Pack of Planets in Alien Solar System
  7. ↑ Michael Mewhinney; Rachel Hoover; Trent J. Perrotto (2 February 2011). "NASA's Kepler Spacecraft Discovers Extraordinary New Planetary System". NASA. Retrieved 4 February 2011.
  8. ↑ Fraser Cain (16 September 2008). "How Old is the Sun?". Universe Today. Retrieved 19 February 2011.
  9. ↑ Fraser Cain (September 15, 2008). "Temperature of the Sun". Universe Today. Retrieved 19 February 2011.
  10. ↑ Boyle, Alan (2 February 2011). "Planetary six-pack poses a puzzle". MSNBC Cosmic Log. Retrieved 4 February 2011.
  11. 1 2 Lissauer, J.; at al. (2013). "All Six Planets Known to Orbit Kepler-11 Have Low Densities". The Astrophysical Journal. 770 (2): id. 131 (15 pp.). arXiv:1303.0227Freely accessible. Bibcode:2013ApJ...770..131L. doi:10.1088/0004-637X/770/2/131.
  12. 1 2 3 4 D'Angelo, G.; Bodenheimer, P. (2016). "In Situ and Ex Situ Formation Models of Kepler 11 Planets". The Astrophysical Journal. 828 (1): id. 33 (32 pp.). arXiv:1606.08088Freely accessible. Bibcode:2016ApJ...828...33D. doi:10.3847/0004-637X/828/1/33.
  13. 1 2 Naeye, Robert (2 February 2011). "Kepler's Outrageous System of Six Planets". Sky & Telescope. Retrieved 4 February 2011.
  14. ↑ John Matson (2 February 2011). "A Wealth of Worlds: Kepler Spacecraft Finds 6 New Exoplanets and Hints at 1,200 More". Scientific American. Retrieved 20 February 2011.
Wikimedia Commons has media related to Kepler-11.

Coordinates: 19h 48m 27.62s, +41° 54′ 32.9″

This article is issued from Wikipedia - version of the 12/2/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.