TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs

Tomer Holczer, Avi Shporer, Tsevi Mazeh, Daniel Fabrycky, Gil Nachmani, Amy McQuillan, Roberto Sanchis-Ojeda, Jerome A. Orosz, William F. Welsh, Eric B. Ford, Daniel Jontof-Hutter

Research output: Contribution to journalArticle

11 Citations (Scopus)

Abstract

Mazeh et al. have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the Kepler mission to distinguish between the prograde and retrograde motion of their orbits with respect to their parent stars' rotation. The approach utilizes TTVs induced by spot-crossing events that occur when the planet moves across a spot on the stellar surface, looking for a correlation between the derived TTVs and the stellar brightness derivatives at the corresponding transits. This can work even in data that cannot temporally resolve the spot-crossing events themselves. Here, we apply this approach to the Kepler KOIs, identifying nine systems where the photometric spot modulation is large enough and the transit timing accurate enough to allow detection of a TTV-brightness-derivatives correlation. Of those systems, five show highly significant prograde motion (Kepler-17b, Kepler-71b, KOI-883.01, KOI-895.01, and KOI-1074.01), while no system displays retrograde motion, consistent with the suggestion that planets orbiting cool stars have prograde motion. All five systems have impact parameter , and all systems within that impact parameter range show significant correlation, except HAT-P-11b where the lack of a correlation follows its large stellar obliquity. Our search suffers from an observational bias against detection of high impact parameter cases, and the detected sample is extremely small. Nevertheless, our findings may suggest that stellar spots, or at least the larger ones, tend to be located at low stellar latitude, but not along the stellar equator, similar to the Sun.

Original languageEnglish (US)
Article number170
JournalAstrophysical Journal
Volume807
Issue number2
DOIs
StatePublished - Jul 10 2015

Fingerprint

transit
planets
planet
time measurement
brightness
Kepler mission
cool stars
obliquity
display devices
equators
suggestion
orbits
modulation
stars
parameter
detection

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Holczer, Tomer ; Shporer, Avi ; Mazeh, Tsevi ; Fabrycky, Daniel ; Nachmani, Gil ; McQuillan, Amy ; Sanchis-Ojeda, Roberto ; Orosz, Jerome A. ; Welsh, William F. ; Ford, Eric B. ; Jontof-Hutter, Daniel. / TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs. In: Astrophysical Journal. 2015 ; Vol. 807, No. 2.
@article{77f93c66c6914c66b18c1891f91c7c0f,
title = "TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs",
abstract = "Mazeh et al. have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the Kepler mission to distinguish between the prograde and retrograde motion of their orbits with respect to their parent stars' rotation. The approach utilizes TTVs induced by spot-crossing events that occur when the planet moves across a spot on the stellar surface, looking for a correlation between the derived TTVs and the stellar brightness derivatives at the corresponding transits. This can work even in data that cannot temporally resolve the spot-crossing events themselves. Here, we apply this approach to the Kepler KOIs, identifying nine systems where the photometric spot modulation is large enough and the transit timing accurate enough to allow detection of a TTV-brightness-derivatives correlation. Of those systems, five show highly significant prograde motion (Kepler-17b, Kepler-71b, KOI-883.01, KOI-895.01, and KOI-1074.01), while no system displays retrograde motion, consistent with the suggestion that planets orbiting cool stars have prograde motion. All five systems have impact parameter , and all systems within that impact parameter range show significant correlation, except HAT-P-11b where the lack of a correlation follows its large stellar obliquity. Our search suffers from an observational bias against detection of high impact parameter cases, and the detected sample is extremely small. Nevertheless, our findings may suggest that stellar spots, or at least the larger ones, tend to be located at low stellar latitude, but not along the stellar equator, similar to the Sun.",
author = "Tomer Holczer and Avi Shporer and Tsevi Mazeh and Daniel Fabrycky and Gil Nachmani and Amy McQuillan and Roberto Sanchis-Ojeda and Orosz, {Jerome A.} and Welsh, {William F.} and Ford, {Eric B.} and Daniel Jontof-Hutter",
year = "2015",
month = "7",
day = "10",
doi = "10.1088/0004-637X/807/2/170",
language = "English (US)",
volume = "807",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "IOP Publishing Ltd.",
number = "2",

}

Holczer, T, Shporer, A, Mazeh, T, Fabrycky, D, Nachmani, G, McQuillan, A, Sanchis-Ojeda, R, Orosz, JA, Welsh, WF, Ford, EB & Jontof-Hutter, D 2015, 'TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs', Astrophysical Journal, vol. 807, no. 2, 170. https://doi.org/10.1088/0004-637X/807/2/170

TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs. / Holczer, Tomer; Shporer, Avi; Mazeh, Tsevi; Fabrycky, Daniel; Nachmani, Gil; McQuillan, Amy; Sanchis-Ojeda, Roberto; Orosz, Jerome A.; Welsh, William F.; Ford, Eric B.; Jontof-Hutter, Daniel.

In: Astrophysical Journal, Vol. 807, No. 2, 170, 10.07.2015.

Research output: Contribution to journalArticle

TY - JOUR

T1 - TIME VARIATION of KEPLER TRANSITS INDUCED by STELLAR SPOTS - A WAY to DISTINGUISH between PROGRADE and RETROGRADE MOTION. II. APPLICATION to KOIs

AU - Holczer, Tomer

AU - Shporer, Avi

AU - Mazeh, Tsevi

AU - Fabrycky, Daniel

AU - Nachmani, Gil

AU - McQuillan, Amy

AU - Sanchis-Ojeda, Roberto

AU - Orosz, Jerome A.

AU - Welsh, William F.

AU - Ford, Eric B.

AU - Jontof-Hutter, Daniel

PY - 2015/7/10

Y1 - 2015/7/10

N2 - Mazeh et al. have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the Kepler mission to distinguish between the prograde and retrograde motion of their orbits with respect to their parent stars' rotation. The approach utilizes TTVs induced by spot-crossing events that occur when the planet moves across a spot on the stellar surface, looking for a correlation between the derived TTVs and the stellar brightness derivatives at the corresponding transits. This can work even in data that cannot temporally resolve the spot-crossing events themselves. Here, we apply this approach to the Kepler KOIs, identifying nine systems where the photometric spot modulation is large enough and the transit timing accurate enough to allow detection of a TTV-brightness-derivatives correlation. Of those systems, five show highly significant prograde motion (Kepler-17b, Kepler-71b, KOI-883.01, KOI-895.01, and KOI-1074.01), while no system displays retrograde motion, consistent with the suggestion that planets orbiting cool stars have prograde motion. All five systems have impact parameter , and all systems within that impact parameter range show significant correlation, except HAT-P-11b where the lack of a correlation follows its large stellar obliquity. Our search suffers from an observational bias against detection of high impact parameter cases, and the detected sample is extremely small. Nevertheless, our findings may suggest that stellar spots, or at least the larger ones, tend to be located at low stellar latitude, but not along the stellar equator, similar to the Sun.

AB - Mazeh et al. have presented an approach that can, in principle, use the derived transit timing variation (TTV) of some transiting planets observed by the Kepler mission to distinguish between the prograde and retrograde motion of their orbits with respect to their parent stars' rotation. The approach utilizes TTVs induced by spot-crossing events that occur when the planet moves across a spot on the stellar surface, looking for a correlation between the derived TTVs and the stellar brightness derivatives at the corresponding transits. This can work even in data that cannot temporally resolve the spot-crossing events themselves. Here, we apply this approach to the Kepler KOIs, identifying nine systems where the photometric spot modulation is large enough and the transit timing accurate enough to allow detection of a TTV-brightness-derivatives correlation. Of those systems, five show highly significant prograde motion (Kepler-17b, Kepler-71b, KOI-883.01, KOI-895.01, and KOI-1074.01), while no system displays retrograde motion, consistent with the suggestion that planets orbiting cool stars have prograde motion. All five systems have impact parameter , and all systems within that impact parameter range show significant correlation, except HAT-P-11b where the lack of a correlation follows its large stellar obliquity. Our search suffers from an observational bias against detection of high impact parameter cases, and the detected sample is extremely small. Nevertheless, our findings may suggest that stellar spots, or at least the larger ones, tend to be located at low stellar latitude, but not along the stellar equator, similar to the Sun.

UR - http://www.scopus.com/inward/record.url?scp=84937019600&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84937019600&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/807/2/170

DO - 10.1088/0004-637X/807/2/170

M3 - Article

VL - 807

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 170

ER -