text: K2 Kepler's Second Mission 1 K2 - a 2-wheel Kepler mission; The second highest peak in the world, a worthy ascent Steve B. Howell NASA Ames Research Center. - ppt download
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  Presentation on theme: "K2 Kepler's Second Mission 1 K2 - a 2-wheel Kepler mission; The second highest peak in the world, a worthy ascent Steve B. Howell NASA Ames Research Center."— Presentation transcript:
  1 K2 Kepler's Second Mission 1 K2 - a 2-wheel Kepler mission; The second highest peak in the world, a worthy ascent Steve B. Howell NASA Ames Research Center
  2 K2 Mission History  Kepler's 2 nd reaction wheel failed in May 2014  ~1 year ago proto-K2 started: white papers out, on- orbit tests conducted  Submitted NASA senior review proposal – Jan 2014  Senior review approved K2 mission for 2-4 years  K2 mission performed first test campaign - March-May 2014  K2 mission officially started 1 June 2014 2
  3 K2 Mission Assets  Telescope already in space  Heliocentric orbit  Large field of view – many targets  Long, uninterrupted time on targets  High precision photometry  Faint sources due to 1-m aperture  Experienced personnel 3
  4 K2 – How it works 4 Spacecraft pointing limited by power and sun angle constraints Solar pressure 50 micronewtons/m^2
  5 K2 mission concept Ecliptic plane pointings allow the K2 mission to balance high-impact science, technical feasibility, and cost  Observe ~4 different fields per year (~80-day campaigns)  New science enabled by various galactic locations  Observe 10,000-20,000 targets per field  Great photometric precision  No exclusive use period  Data to public archive 5
  6 CONCLUSION Fine-point operations provide photometric precision to within a factor of 2 of the Kepler mission The mode of the noise distribution for K2 fine- point data is: K2 Senior Review Orals – 1 April 20146 Photometric Precision in Fine Point SPACECRAFT HEALTH STATUS & COMMUNITY INVOLVEMENT PROGRESS & SCIENCE IMPLICATIONS OVERVIEW
  7 Current State of K2 Photometry  Module 3 died early on, Module 7 died Jan-Feb 2014  K2 will deliver calibrated pixel files first and light curves sometime later in this fiscal year.  A number of groups are already working to make K2 light curves: K2 project, J. Johnson's group, S. Aigrain's group, NexSci (Jessie C.), …..  Telescope pointing will further improve in campaign 3, leading to better photometry  Current state: ~150 ppm 30-min data, ~45 ppm 6.5 hr avg. (12 magnitude star)
  8 K2 C0 "CDPP-like" Results
  9 Photometric Location Log "CDPP"
  10 K2 Campaign Fields 10 Steve Howell K2 ecliptic pointings in the first two years cover northern and southern sky, high and low galactic latitude, 10X greater sky coverage than Kepler mission. K2 fields highlight star clusters, star forming regions, extragalactic fields, including science not available with Kepler.
  11 CONCLUSION Surveying the Ecliptic K2 Senior Review Orals – 1 April 201411 SPACECRAFT HEALTH STATUS & COMMUNITY INVOLVEMENT PROGRESS & SCIENCE IMPLICATIONS OVERVIEW Pleiades & Hyades Upper Sco
  12 K2 Campaign Fields  02014 Apr 3006:33:11.14+21:35:16.4  12014 Jul 2211:35:45.51+01:25:02.3  22014 Oct 1416:24:30.34-22:26:50.3  32015 Jan 0522:26:39.68-11:05:48.0  42015 Mar 2903:56:18.22+18:39:38.1  52015 Jun 2008:40:37.84+16:49:46.6  62015 Sep 1114:01:11.20-13:16:02.8  72015 Dec 0319:34:16.22-22:38:23.4  82016 Feb 2401:04:43.18+05:11:52.2  92016 May 1718:23:35.72-24:12:12.8 +Velocity Vector http://keplerscience.arc.nasa.gov/K2/MissionConcept.shtml#fields
  15 Special microlens campaign
  16 K2 Key Science Cases Transiting Exoplanets – Star Clusters – Star Forming regions  Exoplanets orbiting low-mass stars  ~4000 M stars/field; 100's small planets, dozens in HZ  Exoplanets orbiting bright stars (R<12)  Detect ~50 short period, rocky planets per year  Refine ice to rock boundary  Early targets for TESS, CHEOPS, JWST  Exoplanets orbiting young stars & pre-MS stars  Detection and characterization statistics for this previously unobserved population 16
  17 Exoplanets: Bright Stars 17 K2 transit detection will discover about 50 rocky planets per year.
  18 Exoplanets: M stars 18 K2 will find large and small exoplanets and detect rocky planets within the habitable zone of M stars.
  19 CONCLUSION K2 Senior Review Orals – 1 April 2014 19 WASP 28b – Model Equals Reality K2 light curve – injected JupiterK2 light curve of WASP 28b Injected transit model confirmed by real observation SPACECRAFT HEALTH STATUS & COMMUNITY INVOLVEMENT PROGRESS & SCIENCE IMPLICATIONS OVERVIEW Time (days)
  20 CONCLUSION K2 Senior Review Orals – 1 April 201420 Asteroseismology Yields Stellar Properties of Giant Stars SPACECRAFT HEALTH STATUS & COMMUNITY INVOLVEMENT PROGRESS & SCIENCE IMPLICATIONS OVERVIEW More Evolved Less Evolved
  21 K2 Key Science Cases Extragalactic Observations AGN Variability Study accretion disk behavior and energy reprocessing SN light curves - progenitors Time 0+ light curves serendipitously observed Study shock break-out, model physics 21 Olling et al., 2014
  22 K2 Key Science Cases Microlensing K2 could perform the first microlens parallax measurement Many imaged lens events possible 22 Light curves at Earth and K2 Gould and Horne, 2013
  23 K2: First Light Image Current Status  Scorpius Imaged by K2 December 2013  Campaign 0 – March-May 2014, Calibrated pixel data public  Campaign 1 – June-Aug 2014 First science campaign, data in hand – cal pixel data public in 75 days  Campaign 2 started 22 Aug 2014 23
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