Misplaced Pages

Kilodegree Extremely Little Telescope: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 04:50, 11 December 2013 editKConWiki (talk | contribs)Autopatrolled, Extended confirmed users188,559 edits KELT-North← Previous edit Revision as of 01:25, 26 January 2014 edit undoArtman40 (talk | contribs)2,039 edits Exoplanet Discoveries: Added tableNext edit →
Line 46: Line 46:
== Exoplanet Discoveries == == Exoplanet Discoveries ==


KELT has made four exoplanet discoveries to date. KELT has made three exoplanet and one brown dwarf discoveries to date.


{| class="toccolours sortable" border=1 cellspacing=0 cellpadding=2 align=center style="text-align:center; border-collapse:collapse; margin-left: 0; margin-right: 0;"
* ]
|- bgcolor="#a0b0ff"
* ]
* ] ! ]
* ] ! ]
! ]
! ]
! ]
! ] <small>(])</small>
! ]
! ]
! ]<br /><small>(])</small>
! ]<br/><small>(])</small>
! ] <br/><small>(g/cm<sup>3</sup>)</small>
! ]<br /><small>(])</small>
! ]<br /><small>(])</small>
! ]
! ]<br /><small>(])</small>
! Discovery<br />year
|-
| ] || || {{RA|06|10|39}} || {{DEC|+30|57|26}} || 8.7 || 420 || F7V
| ] || 1.486 || 1.306 || || 4.11379 || 0.05498 || 0.185 ± 0.08) || || 2012
|-
| ] || || {{RA|09|54|34.0}} || {{DEC|+30|38|24}} || 9.8 || || F
| ] || 1.418 || 1.333 || || 2.70339 || 0.04117 || || 84.32 || 2012
|-
| ]|| || {{RA|13|03|56}} || {{DEC|+30|38|24}} || 10.38 || || F
| ] || 0.43 || 1.19 || || 7.84563 || 0.079 || 0.22 {{±|0.01|0.019}} || || 2013
|}


In addition, the survey has discovered brown dwarfs like ].


== References == == References ==

Revision as of 01:25, 26 January 2014

This article needs additional citations for verification. Please help improve this article by adding citations to reliable sources. Unsourced material may be challenged and removed.
Find sources: "Kilodegree Extremely Little Telescope" – news · newspapers · books · scholar · JSTOR (November 2013) (Learn how and when to remove this message)

The Kilodegree Extremely Little Telescope (or KELT) consists of two robotic telescopes that are conducting a survey for transiting exoplanets around bright stars. The project is jointly administered by members of the Ohio State University Department of Astronomy, the Vanderbilt University Department of Physics and Astronomy Astronomy Group, the Lehigh University Department of Physics, and the South African Astronomical Observatory (SAAO).

KELT Telescopes

KELT consists of two telescopes, KELT-North in Arizona in the United States, and KELT-South at the SAAO observing station near Sutherland, South Africa.

Each KELT telescope consists of a wide field (26 degrees by 26 degrees) medium format telephoto lens with a 4.2 cm aperture, mounted in from of a 4k x 4k Apogee CCD. KELT-North uses an Apogee AP16E camera, while KELT South uses an Apogee U16M. The optical assemblies and cameras are mounted on Paramount ME mounts manufactured by Software Bisque.

KELT-North

KELT-North is located at Winer Observatory in southeastern Arizona, about an hour's drive from Tucson. KELT-North was installed at Winer in 2005, and has been operating continuously since then, with occasional interruptions for equipment failures and poor weather.

KELT-South

KELT-South is located at the Sutherland astronomical observation station owned and operated by SAAO, about 370 kilometers (230 mi) North of Cape Town. KELT-South was deployed at Sutherland in 2009.

Science Goals

KELT is dedicated to discovering transiting exoplanets orbiting stars in the brightness range of 8 < V < 10 magnitude. This is the regime just fainter than the set of stars comprehensively surveyed for planets by the radial-velocity surveys, but brighter than those typically observed by most transit surveys.

Operations

Both KELT telescopes operate by sequentially observing a series of pre-defined fields around the sky all night, every night when the weather is good. All exposures are taken with 150-second exposures, optimized to observe stars in the target magnitude range of KELT.

Exoplanet Discoveries

KELT has made three exoplanet and one brown dwarf discoveries to date.

Star Constellation Right
ascension
Declination App.
mag.
Distance (ly) Spectral
type
Planet Mass
(MJ)
Radius
(RJ)
Density
(g/cm)
Orbital
period

(d)
Semimajor
axis

(AU)
Orbital
eccentricity
Inclination
(°)
Discovery
year
KELT-2A 06 10 39 +30° 57′ 26″ 8.7 420 F7V KELT-2Ab 1.486 1.306 4.11379 0.05498 0.185 ± 0.08) 2012
KELT-3 09 54 34.0 +30° 38′ 24″ 9.8 F KELT-3b 1.418 1.333 2.70339 0.04117 84.32 2012
KELT-6 13 03 56 +30° 38′ 24″ 10.38 F KELT-6b 0.43 1.19 7.84563 0.079 0.22
−0.019
2013


In addition, the survey has discovered brown dwarfs like KELT-1b.

References

  1. "The Ohio State Department of Astronomy".
  2. "Vanderbilt Department of Physics and Astronomy".
  3. "Vanderbilt Astronomy Group".
  4. "The Lehigh Department of Physics".
  5. "South African Astronomical Observatory".
  6. Pepper, Joshua; et al. (2007). "The Kilodegree Extremely Little Telescope (KELT): A Small Robotic Telescope for Large-Area Synoptic Surveys". Astronomical Society of the Pacific. 119 (858): 923. doi:10.1086/521836.
  7. Pepper; et al. (1970). "The KELT-South Telescope". Publications of the Astronomical Society of the Pacific. 124 (913): 230–241. arXiv:1202.1826. Bibcode:2012PASP..124..230P. doi:10.1086/665044. {{cite journal}}: Explicit use of et al. in: |author= (help)
  8. "Paramount ME".
  9. "Software Bisque company page".

External links

Exoplanet search projects
Ground-based

Space missions
Past
Current
Planned
Proposed
Cancelled
Related
Categories: