From Wikipedia, the free encyclopedia
Star in the constellation Hercules
GSC 03089-00929 is a
magnitude 12
star located approximately 757
light-years away in the
constellation of
Hercules . This star is a G type
main sequence star that is similar to but slightly cooler than the
Sun .
[2]
This star is identified in
SIMBAD as a
variable star per the
1SWASP survey.
[6]
The star GSC 03089-00929 is named Pipoltr . The name was selected in the
NameExoWorlds campaign by
Liechtenstein , during the 100th anniversary of the
IAU . In the local dialect of
Triesenberg , Pipoltr is a bright and visible
butterfly .
[7]
[8]
Planetary system
In 2007 the
TrES program found exoplanet
TrES-3b , later named Umbäässa , orbiting this star by using the
transit method .
[9]
The transit timing variation analysis did not reveal any additional planets in the system as of 2020,
[10] and the physical mechanism underlying transit timing variations remains unexplained as in 2022.
[11]
See also
References
^
a
b
c
d Vallenari, A.; et al. (Gaia collaboration) (2023).
"Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1.
arXiv :
2208.00211 .
Bibcode :
2023A&A...674A...1G .
doi :
10.1051/0004-6361/202243940 .
S2CID
244398875 .
Gaia DR3 record for this source at
VizieR .
^
a
b
c
d
e
f
g
h
i
"NAME TrES-3 Parent Star" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2009-04-23 .
^ Lister, T. A.; West, R. G.; Wilson, D. M.; Collier Cameron, A.; Clarkson, W. I.; Street, R. A.; Enoch, B.; Parley, N. R.; et al. (June 30, 2007).
"SuperWASP-North extrasolar planet candidates: candidates from fields 17h<RA<18h" (PDF) . Monthly Notices of the Royal Astronomical Society . 379 (2): 647–662.
arXiv :
0705.2603 .
Bibcode :
2007MNRAS.379..647L .
doi :
10.1111/j.1365-2966.2007.11948.x .
S2CID
14333676 .
^
a
b
c
d
e
f
g Sozzetti, Alessandro; et al. (2009). "A New Spectroscopic and Photometric Analysis of the Transiting Planet Systems TrES-3 and TrES-4". The Astrophysical Journal . 691 (2): 1145–1158.
arXiv :
0809.4589 .
Bibcode :
2009ApJ...691.1145S .
doi :
10.1088/0004-637X/691/2/1145 .
S2CID
3741198 .
^
a
b
c Püsküllü, Ç.; et al. (2017). "Photometric investigation of hot exoplanets: TrES-3b and Qatar-1b". New Astronomy . 55 : 39–47.
arXiv :
1704.03697 .
Bibcode :
2017NewA...55...39P .
doi :
10.1016/j.newast.2017.04.001 .
S2CID
119208251 .
^
"Objects in reference 2007MNRAS.379..647L" .
Centre de Données astronomiques de Strasbourg . Retrieved 2009-05-03 .
^
"Approved names" . NameExoworlds . Archived from
the original on 2019-12-19. Retrieved 2020-01-02 .
^
"International Astronomical Union | IAU" . www.iau.org . Retrieved 2020-01-02 .
^ O'Donovan, Francis T.; Charbonneau, David; Bakos, Gáspár Á.; Mandushev, Georgi; Dunham, Edward W.; Brown, Timothy M.; Latham, David W.; Torres, Guillermo; et al. (July 1, 2007). "TrES-3: A Nearby, Massive, Transiting Hot Jupiter in a 31-Hour Orbit". Astrophysical Journal Letters . 663 (1): L37–L40.
arXiv :
0705.2004 .
Bibcode :
2007ApJ...663L..37O .
doi :
10.1086/519793 .
S2CID
17637874 .
^ Mannaday, Vineet Kumar; Thakur, Parijat; Jiang, Ing-Guey; Sahu, D. K.; Joshi, Y. C.; Pandey, A. K.; Joshi, Santosh; Yadav, Ram Kesh; Su, Li-Hsin; Sariya, Devesh P.; Yeh, Li-Chin; Griv, Evgeny; Mkrtichian, David; Shlyapnikov, Aleksey; Moskvin, Vasilii; Ignatov, Vladimir; Vaňko, M.; Püsküllü, Ç. (2020).
"Probing Transit Timing Variation and Its Possible Origin with 12 New Transits of TrES-3b" . The Astronomical Journal . 160 (1): 47.
arXiv :
2006.00599 .
Bibcode :
2020AJ....160...47M .
doi :
10.3847/1538-3881/ab9818 .
S2CID
219176648 .
^ Mannaday, Vineet Kumar; Thakur, Parijat; Southworth, John; Jiang, Ing-Guey; Sahu, D. K.; Mancini, L.; Vaňko, M.; Kundra, Emil; Gajdoš, Pavol; a-Thano, Napaporn; Sariya, Devesh P.; Yeh, Li-Chin; Griv, Evgeny; Mkrtichian, David; Shlyapnikov, Aleksey (2022), "Revisiting the Transit Timing Variations in the TrES-3 and Qatar-1 Systems with TESS Data", The Astronomical Journal , 164 (5): 198,
arXiv :
2209.04080 ,
Bibcode :
2022AJ....164..198M ,
doi :
10.3847/1538-3881/ac91c2 ,
S2CID
252185524
^ MacKebrandt, F.; et al. (2017). "Transmission spectroscopy of the hot Jupiter TrES-3 b: Disproof of an overly large Rayleigh-like feature". Astronomy and Astrophysics . 608 . A26.
arXiv :
1709.06124 .
Bibcode :
2017A&A...608A..26M .
doi :
10.1051/0004-6361/201730512 .
S2CID
53995250 .
External links