 | Review waiting, please be patient.
This may take 8 weeks or more, since drafts are reviewed in no specific order. There are 1,743 pending submissions waiting for review.
Where to get help
How to improve a draft
You can also browse Wikipedia:Featured articles and Wikipedia:Good articles to find examples of Wikipedia's best writing on topics similar to your proposed article. Improving your odds of a speedy review To improve your odds of a faster review, tag your draft with relevant WikiProject tags using the button below. This will let reviewers know a new draft has been submitted in their area of interest. For instance, if you wrote about a female astronomer, you would want to add the Biography, Astronomy, and Women scientists tags. Editor resources
Reviewer tools
|
| Submission declined on 10 December 2024 by Significa liberdade (talk). This submission appears to be taken from https://anunakiobservatory.es/en/qatar-5b-2/. Wikipedia cannot accept material copied from elsewhere, unless it explicitly and verifiably has been released to the world under a suitably free and compatible copyright license or into the public domain and is written in an acceptable tone—this includes material that you own the copyright to. You should attribute the content of a draft to outside sources, using citations, but copying and pasting or closely paraphrasing sources is not acceptable. The entire draft should be written using your own words and structure.
Where to get help
How to improve a draft
You can also browse Wikipedia:Featured articles and Wikipedia:Good articles to find examples of Wikipedia's best writing on topics similar to your proposed article. Improving your odds of a speedy review To improve your odds of a faster review, tag your draft with relevant WikiProject tags using the button below. This will let reviewers know a new draft has been submitted in their area of interest. For instance, if you wrote about a female astronomer, you would want to add the Biography, Astronomy, and Women scientists tags. Editor resources
This draft has been resubmitted and is currently awaiting re-review. |  |
This submission has now been cleaned of the above-noted copyright violation and its history redacted by an administrator to remove the infringement. If re-submitted (and subsequent additions do not reintroduce copyright problems), the content may be assessed on other grounds.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Andromeda |
| Right ascension | 00h 28m 13.00s[1] |
| Declination | +42° 03′ 41.00″[1] |
| Apparent magnitude (V) | 12.82[2] |
| Characteristics | |
| Evolutionary stage | main sequence star |
| Spectral type | G5V |
| Variable type | planetary transit |
| Astrometry | |
| Proper motion (μ) | RA: 0.919±0.031 mas/yr[1] Dec.: −6.509±0.017 mas/yr[1] |
| Parallax (π) | 2.693 ± 0.035 mas[1] |
| Distance | 1,210 ± 20 ly (371 ± 5 pc) |
| Details | |
| Mass | 1.128±0.056[3] M☉ |
| Radius | 1.076±0.051[3] R☉ |
| Luminosity | 1.13[2] L☉ |
| Surface gravity (log g) | 4.427±0.035[3] cgs |
| Temperature | 5746±49[3] K |
| Metallicity [Fe/H] | 0.38±0.08[3] dex |
| Rotational velocity (v sin i) | 10.4±0.5[2] km/s |
| Age | 5.47±0.1[2] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
Qatar-5 is a faint G-dwarf star that hosts a planet in the constellation Andromeda. With an apparent magnitude of 12.82, it is impossible to detect with the naked eye, but can be detected with a powerful telescope. Qatar-5 is currently located about 1,211 light years away based on parallax.
Properties
editThis star is a relatively young star with an age of only 5.47 billion years. At this age, it is still on the main sequence. Qatar-5 has 112.8% the mass of the Sun, and 107.6% the latter's radius. Despite all of this, it has 113% of the Sun's luminosity, which corresponds to an effective temperature of 5,746 K. Qatar-5 rotates at a rate of 10.4 km/s.
Planetary system
editIn 2016, the Qatar Exoplanet Survey discovered a planet around this star.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 4.32±0.18 MJ | 0.04127±0.00067 | 2.8792319 | 0 | 88.74±0.87° | 1.107±0.064 RJ |
| Discovery[4] | |
|---|---|
| Discovered by | Alsubai et al. 2019 |
| Discovery date | 2016 |
| Transit | |
| Orbital characteristics | |
| 0.04127 ± 0.00067 au[4] | |
| Eccentricity | 0[4] |
| 2.8792319 d[4] | |
| Inclination | 88.74 ± 0.87°[4] |
| Semi-amplitude | 568 ± 15 m/s[4] |
| Physical characteristics | |
| 1.107 ± 0.064 RJ[4] | |
| Mass | 4.32 ± 0.18 MJ[4] |
Mean density | 3.95 ± 0.58 g cm−3[4] |
| Temperature | 1415 ± 31 K[4] |
Qatar-5b
editQatar-5b is a Hot Jupiter orbiting the star Qatar-5 located in Andromeda constellation.[5] It orbits its star every 2.87 days. It was discovered in 2016 by the Qatar Exoplanet Survey (QES).[6][4]
Discovery
editThis planet was discovered by QES along with Qatar-3b and Qatar-4b. The light curves of the planet's respective host stars have been observed as well during the survey, along with their stellar properties[7]
Properties
editOrbit
editThis planet is another typical hot Jupiter. It orbits very close to its star with a period of 2 days, 21 hours, 6 minutes, and 5.6 seconds.[8] This corresponds with an orbital distance of 0.04127 AU, which is about 10 times closer to its star than Mercury is to the Sun. With an eccentricity of 0, this suggests that Qatar-5b is on a perfectly circular orbit.
Physical properties
editQatar-5b is a massive planet, with 4.32 times the mass of Jupiter, but a similar radius. With a density of 3.95 g cm−3, this is one of the densest planets discovered. With an effective temperature of 1,415 K, it is a scorching planet.
See also
editReferences
edit- ^ a b c d Gaia Collaboration (2018-04-01). "VizieR Online Data Catalog: Gaia DR2 (Gaia Collaboration, 2018)". VizieR Online Data Catalog. 1345. Bibcode:2018yCat.1345....0G. doi:10.26093/cds/vizier.1345.
- ^ a b c d Alsubai, Khalid; Mislis, Dimitris; Tsvetanov, Zlatan I.; Latham, David W.; Bieryla, Allyson; Buchhave, Lars A.; Esquerdo, Gilbert A.; Bramich, D. M.; Pyrzas, Stylianos; Vilchez, Nicolas P. E.; Mancini, Luigi (2017-04-01). "Qatar Exoplanet Survey : Qatar-3b, Qatar-4b, and Qatar-5b" (PDF). The Astronomical Journal. 153 (4): 200. arXiv:1606.06882. Bibcode:2017AJ....153..200A. doi:10.3847/1538-3881/aa6340. ISSN 0004-6256. S2CID 119214858.
- ^ a b c d e f Wang, Xian-Yu; Wang, Yong-Hao; Wang, Songhu; Wu, Zhen-Yu; Rice, Malena; Zhou, Xu; Hinse, Tobias C.; Liu, Hui-Gen; Ma, Bo; Peng, Xiyan; Zhang, Hui; Yu, Cong; Zhou, Ji-Lin; Laughlin, Gregory (2021), "Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves", The Astrophysical Journal Supplement Series, 255 (1): 15, arXiv:2105.14851, Bibcode:2021ApJS..255...15W, doi:10.3847/1538-4365/ac0835, S2CID 235253975
- ^ a b c d e f g h i j k Alsubai, Khalid; et al. (2017). "Qatar Exoplanet Survey: Qatar-3b, Qatar-4b, and Qatar-5b". The Astronomical Journal. 153 (4). 200. arXiv:1606.06882. Bibcode:2017AJ....153..200A. doi:10.3847/1538-3881/aa6340. S2CID 119214858.
- ^ "Qatar-5". Universe Guide. 15 September 2018. Retrieved 2019-12-27.
- ^ "Astronomers discover three 'Qatar' exoplanets".
- ^ Alsubai, Khalid; Mislis, Dimitris; Tsvetanov, Zlatan I.; Latham, David W.; Bieryla, Allyson; Buchhave, Lars A.; Esquerdo, Gilbert A.; Bramich, D. M.; Pyrzas, Stylianos; Vilchez, Nicolas P. E.; Mancini, Luigi (2017-04-01). "Qatar Exoplanet Survey : Qatar-3b, Qatar-4b, and Qatar-5b". The Astronomical Journal. 153 (4): 200. arXiv:1606.06882. Bibcode:2017AJ....153..200A. doi:10.3847/1538-3881/aa6340. ISSN 0004-6256.
- ^ "Convert a Decimal Time Amount to Days, Hours, Minutes and Second". www.spikevm.com. Retrieved 2021-03-25.