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Goldilocks Zones – a Fine-Grained Exoplanet Taxonomy Patrick J. Talbot (Presenter) Dennis R. Ellis (Analysis) Introduction and Summary Situation: Since the 1990's, over 5,000 exoplanets have been identified* and the rate of discovery is accelerating: 1,569 Planets with good orbits + 24 Microlensing and imaged planets = 1,593 Total confirmed planets + 3,751 Unconfirmed Kepler candidates = 5,344 Total exoplanets + Kelper Candidates https://github.com/OpenExoplanetCatalogue/open_exop Need: a robust, extensible organization scheme for understanding, processing, and pattern discovery Approach: ● A classic trade study to rank and score candidate attributes ● A critic, a sequential optimizer, and software tests ● Iteration to find a minimum spanning taxonomy Result: ● A minimum spanning taxonomy provides a uniques set of characteristics for each exoplanet. ● To the extent practical, each exoplanet has a unique set of characteristics, or signature. ● * http://exoplanets.org/, as of 1 September 2015. Objective ● ● ● ● ● Organize information about exoplanets Input exoplanets characteristics into a hierarchical, frame-based ontology, like Protege Identify the minimum set of characteristics that span the problem space, so that each exoplanet has, to the extent practical, a unique signature. Input the knowledge base into data analytics tools, such as Weka Rule Induction, to automatically discover interesting pattterns. Quantify missing and conflicting data as sources of uncertainty to drive further refinement Approach ● ● Perform Trades Mission Functional Discretize ● Rules Filter Attributes ● Birthday Problem Compute Signatures Yes Verify Uniqueness No Unique? Reduce #States Increase #States No Yes Minimal? Done Tag Planet Star Binary Declination Rightascension Distance Name Semimajoraxis Separation Positionangle Eccentricity Periastron Longitude Meananomaly Ascendingnode InclinatioN Epoch Period Transittime Periastrontime Mass Radius Temperature Age Metallicity Spectraltype MagB MagV MagR MagI MagJ MagH MagK Discoverymethod Istransiting Description Discoveryyear Lastupdate Spinorbitalignment Data Structures, MIT Open Exoplanet Catalog Description a single planet. May be a free floating (orphan) planet A single star. A star can be host to one or more planets two stars, star/binary or two binaries. Declination Right ascension Distance from the Sun Used multiple times for objects with multiple names. Semi-major axis of a planet (heliocentric coordinates) Projected separation of planet from its host Position angle Eccentricity Longitude of periastron Mean longitude at a given Epoch (all planets in a system) Mean anomaly at a given Epoch (all planets in one system) Longitude of the ascending node Inclination of the orbit Epoch for the orbital elements Orbital period Time of the center of a transit Time of periastron Mass (or m sin(i) for radial velocity planets) Physical radius Temperature (surface or equilibrium) Age Stellar metallicity Spectral type B magnitude Visual magnitude R magnitude I magnitude J magnitude H magnitude K magnitude Discovery method : timing, RV, transit, imaging. Whether the planet is transiting (1) or not (0). Short description of the planet Year of the planet's discovery Date of the last (non-trivial) update Rossiter-McLaughlin Effect. Mission Trade Study Functional Trade Study Node Composite Score Sample Rules Probability of Duplicates vs Catalog Size Exoplanet Characteristics Hierarchy Exoplanet Name Input Header Only Elements Period Exoplanets Header Only Physical Header Only Host star Inclination Metallicity Distance Binary Eccentricity Spectral Type Mass Semi-major axis Radius Separation Age Temperature Exoplanet Signature Separation (Moderate) Distance (Far) Eccentricity (Nearly Circular) Mass (Small) Spectral type (Hottest) Age (Ancient) Temperature (Hot) H H 2 M LS L N L O LA Binary (2 stars) Period (Long) Inclination (Low) Semi-major Axis (Large) Physical Radius (Large) Exoplanet Kiviat Diagram Physical Orbital Composition [FeHg] Inclination Mass Period Size Goldilocks Zone Kepler 423c Habitability Index = .3 Host Variability Host Age Host Spectral Type Environmental Influential Coming in the Full Paper ● Percent of Duplicate Signatures ● Sensitivity of Duplicates to Attribute States ● Optimum Set of Attributes and # States ● Weka Rule Induction to Identify Patterns Summary ● Characteristics of an exoplanet taxonomy were identified ● Trade studies ranked attributes ● Rules discretized attributes ● Taxonomy was sized (Birthday Problem) ● A fine-grained taxonomy was portrayed: ● Taxonomy Hierarchy ● Taxonomy Signature ● Taxonomy Kiviat Backup:Example Histograms