79 Ceti

Short description: Binary star system in the constellation of Cetus

79 Ceti  Observation data
Equinox J2000.0]] (ICRS)

Constellation | Cetus
Right ascension |  02h 35m 19.9293s[1]
Declination | −03° 33′ 38.1707″[1]
Apparent magnitude (V) | +6.83[2]
Characteristics
Spectral type | G2V+M[3][4] or G8IV[5]
B−V color index | 0.670±0.004[2]
Variable type | none
Astrometry
Radial velocity (Rv)| −50.93±0.09[2] km/s
Proper motion (μ)|  RA: −155.58[1] mas/yr
Dec.: −437.99[1] mas/yr
Parallax (π)| 26.4360 ± 0.0580[1] mas
Distance| 123.4 ± 0.3 ly
(37.83 ± 0.08 pc)
Absolute magnitude (MV)| +3.88[2]
Details[6]
79 Ceti A
Mass| 1.01 M☉
Radius| 1.48[7] R☉
Luminosity| 1.99±0.04 L☉
Surface gravity (log g)| 4.19±0.02 cgs
Temperature| 5,806±17 K
Metallicity [Fe/H]| +0.16±0.01[6] dex
Age| 6.0[8] or 9.4±0.8[2] Gyr
79 Ceti B
Mass| 0.286[4] M☉
Other designations

79 Cet, BD−04°426, FK5 4237, Gaia DR2 2495335115182966016, GJ 9085, HD 16141, HIP 12048, SAO 129992, WDS J02353-0334A, 2MASS J02351994-0333376[9]

Database references
SIMBAD| data

79 Ceti, also known as HD 16141, is a binary star system located 123[1] light-years from the Sun in the southern constellation of Cetus. It has an apparent visual magnitude of +6.83,[2] which puts it below the normal limit for visibility with the average naked eye. The star is drifting closer to the Earth with a heliocentric radial velocity of −51 km/s.[2]

Harlan (1974) assigned this star a stellar classification of G2V,[3] matching an ordinary G-type main-sequence star that is undergoing core hydrogen fusion. However, Houk and Swift (1999) found a class of G8IV,[5] which suggests it has exhausted the supply of hydrogen at its core and begun to evolve off the main sequence. Eventually the outer layers of the star will expand and cool and the star will become a red giant. Estimates of the star's age range from 6.0[8] to 9.4 billion years old. It has an estimated 1.06 times the mass of the Sun and 1.48[7] times the Sun's radius. The star is radiating twice[6] luminosity of the Sun from its photosphere at an effective temperature of 5,806 K.[6] The discrepancy was later found to be due to an additional red dwarf star in the system at a projected separation 220 AUs.[4]

## Contents

* 1 Planetary system
* 2 See also
* 3 References
* 4 External links

## Planetary system

On March 29, 2000, a planet orbiting primary star was announced, it was discovered using the radial velocity method.[10] This object has a minimum 0.26 times the mass of Jupiter and is orbiting its host star every 75.5 days.[11]

The 79 Ceti planetary system[12] Companion
(in order from star) | Mass | Semimajor axis
(AU) | Orbital period
(days) | Eccentricity | Inclination | Radius

|
|
|
|
|
|

b | ≥0.260 ± 0.028 MJ | 0.363 ± 0.021  | 75.523 ± 0.055  | 0.252 ± 0.052  | —  | —

## See also

* 81 Ceti
* 94 Ceti
* Lists of exoplanets

## References

1. ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
2. ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A.
3. ↑ 3.0 3.1 Harlan, E. A. (June 1974). "MK classification for F- and G-type stars. III.". Astronomical Journal 79: 682–686. doi:10.1086/111597. Bibcode: 1974AJ.....79..682H.
4. ↑ 4.0 4.1 4.2 Quarles, Billy; Li, Gongjie; Kostov, Veselin; Haghighipour, Nader (2020), "Orbital Stability of Circumstellar Planets in Binary Systems", The Astronomical Journal 159 (3): 80, doi:10.3847/1538-3881/ab64fa, Bibcode: 2020AJ....159...80Q
5. ↑ 5.0 5.1 Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey 5. Bibcode: 1999MSS...C05....0H.
6. ↑ 6.0 6.1 6.2 6.3 S. G., Sousa et al. (August 2008). "Spectroscopic parameters for 451 stars in the HARPS GTO planet search program. Stellar [Fe/H] and the frequency of exo-Neptunes". Astronomy and Astrophysics 487 (1): 373–381. doi:10.1051/0004-6361:200809698. Bibcode: 2008A&A...487..373S.
7. ↑ 7.0 7.1 Stassun, Keivan G. et al. (March 2017). "Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes". The Astronomical Journal 153 (3): 20. doi:10.3847/1538-3881/aa5df3. 136. Bibcode: 2017AJ....153..136S.
8. ↑ 8.0 8.1 Sousa, S. G. et al. (March 2010). "Higher depletion of lithium in planet host stars: no age and mass effect". Astronomy and Astrophysics 512: L5. doi:10.1051/0004-6361/201014125. Bibcode: 2010A&A...512L...5S.
9. ↑ "79 Cet". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=79+Cet.
10. ↑ "Keck astronomers discover planets smaller than saturn" (Press release). Kamuela, Hawaii: W. M. Keck Observatory. March 29, 2000. Retrieved August 13, 2019.
11. ↑ Marcy, Geoffrey W. et al. (2000). "Sub-Saturn Planetary Candidates of HD 16141 and HD 46375". The Astrophysical Journal Letters 536 (1): L43–L46. doi:10.1086/312723. PMID 10849416. Bibcode: 2000ApJ...536L..43M.
12. ↑ Butler, J. T. et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505–522. doi:10.1086/504701. Bibcode: 2006ApJ...646..505B.

## External links

* SIMBAD: HD 16141 -- High proper-motion Star
* SolStation: 79 Ceti
* Extrasolar Planets Encyclopaedia: HD 16141

Coordinates:  02h 35m 19.9283s, −03° 33′ 38.167″

* v
* t
* e

Cetus constellation

Stars
(list)|

| Bayer|

* α (Menkar)
* β (Diphda)
* γ (Kaffaljidhma)
* δ
* ε
* ζ (Baten Kaitos)
* η
* θ
* ι
* κ1
* κ2
* λ
* μ
* ν
* ξ1
* ξ2
* ο (Mira)
* π
* ρ
* σ
* τ
* υ
* φ1
* φ2
* φ3
* φ4
* χ

|

Flamsteed|

* 1
* 2
* 3
* 6
* 7
* 9
* 10
* 11
* 12
* 13
* 14
* 15
* 18
* 20
* 21
* 25
* 26
* 27
* 28
* 29
* 30
* 32
* 33
* 34
* 35
* 36
* 37
* 38
* 39
* 40
* 41
* 42
* 43
* 44
* 46
* 47
* 48
* 49
* 50
* 56
* 57
* 58
* 60
* 61
* 62
* 63
* 64
* 66
* 67
* 69
* 70
* 71
* 75
* 77
* 79
* 80
* 81
* 84
* 93
* 94
* 95
* 25 Ari

Variable|

* T
* RR
* TV
* TW
* UU
* VZ (Mira B)
* WW
* WX
* XY
* XZ
* YZ
* ZZ
* AA
* AB
* AD
* AR
* BG
* BK
* CF
* DK
* EH
* EL
* EO
* ES

HR|

* 9
* 10
* 12
* 16
* 31
* 37
* 51
* 61
* 66
* 72
* 108
* 115
* 118
* 150
* 159
* 172
* 173
* 174
* 190
* 197
* 201
* 206
* 210
* 218
* 220
* 227
* 228
* 232
* 247
* 251
* 263
* 320
* 325
* 387
* 388
* 392
* 394
* 404
* 405
* 406
* 416
* 425
* 448
* 466
* 473
* 492
* 500
* 507
* 513
* 560
* 608
* 611
* 616
* 625
* 638
* 651
* 672
* 684
* 692
* 693
* 697
* 713
* 719
* 725
* 732
* 735
* 737
* 745
* 751
* 766
* 770
* 775
* 783
* 784
* 795
* 796
* 816
* 870
* 908
* 926
* 942
* 9054
* 9095
* 9096
* 9101

HD|

* 1690
* 1879
* 2268
* 2638
* 4747
* 5319
* 6037
* 6718
* 7449
* 8713
* 8896
* 9690
* 9731
* 10024
* 10725
* 11365
* 11396
* 11506
* 11964
* 12116
* 12702
* 13004
* 13546
* 13763
* 15115
* 16008
* 16031
* 17001
* 224349
* 224693 (Axólotl)

Gliese|

* Gliese 40
* Gliese 105
* GJ 1002
* GJ 1005
* GJ 1057
* GJ 2012

Other|

* BD−17 63
* Cayrel's Star
* CFBDS J005910.90–011401.3
* CS 31082-001
* DENIS-P J020529.0−115925
* GD 40
* HIP 5158
* HIP 11952
* L 870-2
* LHS 1140
* Luyten 726-8 (UV/BL)
* NGC 156
* NGC 302
* NGC 308
* NGC 310
* PSR B0031−07
* PSR J0034−0534
* PSR J0108−1431
* SDSS J001820.5−093939.2
* SDSS J0106−1000
* ULAS J003402.77−005206.7
* WD J2356-209
* WASP-26
* WASP-44
* WASP-71
* WISE J0254+0223

Nebulae|

| Planetary|

* BoBn 1
* NGC 246

|

Galaxies|

| Messier|

* 77

|

NGC|

* 17
* 35
* 45
* 47
* 50
* 54
* 59
* 61
* 62
* 64
* 65
* 66
* 73
* 77
* 102
* 107
* 113
* 114
* 117
* 118
* 120
* 124
* 132
* 135
* 142
* 143
* 144
* 145
* 151
* 154
* 155
* 157
* 161
* 163
* 165
* 166
* 167
* 168
* 170
* 171
* 172
* 173
* 177
* 178
* 179
* 187
* 191
* 192
* 195
* 196
* 197
* 201
* 207
* 209
* 210
* 216
* 217
* 219
* 223
* 227
* 230
* 232
* 235A
* 235B
* 237
* 239
* 244
* 245
* 247
* 255
* 259
* 263
* 268
* 270
* 271
* 273
* 274
* 275
* 276
* 277
* 279
* 283
* 284
* 285
* 286
* 291
* 293
* 297
* 298
* 301
* 303
* 307
* 309
* 320
* 321
* 325
* 327
* 329
* 331
* 333
* 333B
* 335
* 336
* 337
* 337A
* 340
* 341
* 341B
* 342
* 343
* 344
* 345
* 347
* 349
* 350
* 351
* 352
* 353
* 355
* 356
* 357
* 359
* 363
* 364
* 367
* 369
* 377
* 391
* 413
* 417
* 426
* 428
* 429
* 430
* 435
* 442
* 445
* 448
* 450
* 478
* 480
* 481
* 487
* 493
* 497
* 519
* 521
* 530
* 533
* 535
* 538
* 539
* 540
* 541
* 543
* 545
* 547
* 548
* 550
* 554A
* 554B
* 555
* 556
* 557
* 558
* 560
* 564
* 565
* 567
* 570
* 577
* 578
* 583
* 584
* 585
* 586
* 589
* 593
* 594
* 596
* 599
* 600
* 601
* 615
* 617
* 622
* 624
* 635
* 636
* 640
* 647
* 648
* 649
* 655
* 667
* 681
* 682
* 690
* 699
* 701
* 702
* 707
* 713
* 715
* 720
* 725
* 726
* 731
* 734
* 747
* 748
* 755
* 756
* 758
* 762
* 767
* 768
* 773
* 779
* 787
* 788
* 790
* 799
* 800
* 806
* 808
* 809
* 811
* 814
* 815
* 825
* 827
* 829
* 830
* 831
* 833
* 835
* 836
* 837
* 838
* 839
* 840
* 842
* 844
* 848
* 849
* 850
* 851
* 853
* 858
* 859
* 863
* 864
* 867
* 868
* 872
* 873
* 874
* 878
* 879
* 880
* 881
* 883
* 887
* 892
* 894
* 895
* 899
* 902
* 905
* 907
* 908
* 921
* 926
* 929
* 934
* 936
* 941
* 942
* 943
* 944
* 945
* 947
* 948
* 950
* 951
* 955
* 958
* 960
* 963
* 965
* 966
* 967
* 975
* 977
* 981
* 985
* 988
* 989
* 991
* 993
* 997
* 998
* 1004
* 1007
* 1008
* 1009
* 1010
* 1011
* 1013
* 1015
* 1016
* 1017
* 1018
* 1019
* 1020
* 1021
* 1022
* 1026
* 1032
* 1033
* 1034
* 1035
* 1038
* 1041
* 1042
* 1043
* 1044
* 1045
* 1046
* 1047
* 1048
* 1048A
* 1051
* 1052
* 1055
* 1063
* 1064
* 1065
* 1069
* 1070
* 1071
* 1072
* 1073
* 1074
* 1075
* 1076
* 1078
* 1080
* 1085
* 1087
* 1090
* 1094
* 1095
* 1101
* 1104
* 1105
* 1107
* 1128
* 1137
* 1141
* 1142
* 1149
* 1153
* 1194
* 1211
* 1218
* 1219
* 1254
* 1280
* 7807
* 7808
* 7813
* 7821
* 7828
* 7829

Other|

* Arp 147
* Arp 256
* 3C 15
* 3C 17
* 3C 75
* Cetus Dwarf Spheroidal galaxy
* HCM-6A
* Holmberg 15A
* IC 1613
* IRAS F01475-0740
* Markarian 573
* Markarian 1014
* Markarian 1018
* Markarian 1044
* NAB 0205+024
* PHL 938
* PKS 0048-097
* PKS 0106+013
* PKS 0119-046
* PKS 0139-097
* PKS 0215+015
* PKS 0237-233
* PKS 0306+102
* QSO B0137+012
* QSO B0302-003
* SDSS J0303-0019
* SMM J02399-0136
* SXDF-NB1006-2
* 9Spitch
* Ton S180
* UM 673
* VV 114
* Wolf–Lundmark–Melotte

Galaxy
clusters|

* Abell 85
* Abell 119
* Abell 133
* Abell 151
* Abell 168
* Abell 194
* Abell 209
* Abell 222
* Abell 223
* Abell 267
* Abell 370
* Abell 400
* HCG 16
* IRC 0218
* JKCS 041
* RX J0152.7-1357

Other|

* GRB 000911
* GRB 041006
* GRB 050908
* GRB 060908
* GRB 091127
* SN 1984L
* SN 2005gj
* SN 2005hk

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