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HD 86065 Overview

HD 86065 0.78 R⦿ 4927.56 K
HD 86065 b
Architecture
HD 86065
HD 86065
HD 86065 b
Other Data
Bibliography 2
Nearby Data 3
Discovery Data
Host Planet Method Year Reference Disposition
HD 86065 HD 86065 b Radial Velocity 2022 Feng et al. 2022 Confirmed Planet
RA
09h55m42.16s
Dec
-18d06m24.98s
Distance
40.3661+0.0557-0.0555
pc
Parallax
24.7443000±0.0338969 mas
Ecliptic Latitude
-28.70438 deg
Ecliptic Longitude
158.14331 deg
Galactic Latitude
27.86969 deg
Galactic Longitude
254.68749 deg
Total Proper Motion
343.7497904±0.0629830 mas/yr
Proper Motion (RA)
-326.1880000±0.0615423 mas/yr
Proper Motion (Dec)
108.4680000±0.0747617 mas/yr
Photometry
mV
9.36±0.03
mTESS
8.4743±0.0060
mJ
7.650±0.027
mH
7.183±0.042
mKs
7.086±0.018
mGaia
9.060590±0.000707
mB
10.302±0.091
Abundances
(Hypatia Catalog)
[Fe/H] 0.01±0.09 dex
[C/H] 0.06±0.19 dex
[O/H] 0.07±0.09 dex
[Na/H] 0.04±0.03 dex
[Mg/H] 0.04±0.08 dex
[Al/H] 0.11±0.02 dex
[Si/H] 0.04±0.10 dex
[Ca/H] 0.00±0.06 dex
[BaII/H] 0.07±0.06 dex
Tools
ExoFOP Target Overview Page
IRSA Finding Chart
Stellar Hosts
Source Feng et al. 2022 TICv8
M✶
(M⦿)
0.810±0.092
0.8100000+0.1112960-0.0731916
Teff
(K)
---
4927.5600+111.2120-93.8655
L✶
(log10(L⦿))
---
-0.4902024+0.0143842-0.0081832
Metallicity
(dex)
--- -0.0201639±0.0153644 [M/H]
ρ✶
(g/cm3)
---
2.403190+0.654592-0.396741
R✶
(R⦿)
---
0.7803470+0.0492085-0.0358618
log g
(log10(cm/s2))
---
4.5619800+0.0782175-0.0782979
Print
Status
Confirmed Planet
Detected By
Radial Velocity
Tools
Source Feng et al. 2022
Tp
(days)
2433116.260+16957.054-9561.935
ω
(deg)
142.418+140.159-56.450
Mp
(M⨁)
2877.3+855.0-815.9
Mp
(MJup)
9.0530+2.6900-2.5670
e
0.2190+0.1560-0.1520
i
(deg)
29.821+17.890-17.334
P
(days)
25775.78859+13279.46721-9595.00303
K
(m/s)
36.389+0.428-21.795
a
(au)
15.947+4.799-4.381
Print
Known Objects
1 Confirmed Planets
2 2MASS Point Source Catalog
Data Files
1 Associated Literature Data
System
Star
Confirmed
Candidate
False Positive Planet
Controversial
False Positive
Aliases
Data Access
Transit Prediction Service
Time Series
Kepler | K2
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