Orbital parameter of exoplanets detected around HD 69830. The source of the values in the table (Ref) is given in the final column: 1.(Laliotis et al. 2023), 2. This study.
Planet . | Parameter . | Best fit . | Ref . |
---|---|---|---|
P(d) | |$8.66897\pm 0.00028$| | 1 | |
e | |$0.128\pm 0.028$| | 1 | |
HD 69830 b | K(m s−1) | |$3.4\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$10.1^{+0.38}_{-0.37}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.14^{+1.75}_{-0.34}$| | 2 | |
Orbital distance (AU) | |$0.079\pm 0.001$| | 2 | |
P(d) | |$31.6158\pm 0.0051$| | 1 | |
e | |$0.03\pm 0.03$| | 1 | |
HD 69830 c | K (m s−1) | |$2.6\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.09^{+0.55}_{-0.54}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.12}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.188\pm 0.001$| | 2 | |
P (d) | |$201.4\pm 0.4$| | 1 | |
e | |$0.08\pm 0.07$| | 1 | |
HD 69830 d | K (m s−1) | |$1.5\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.26^{+0.89}_{-0.88}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.17}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.644\pm 0.001$| | 2 |
Planet . | Parameter . | Best fit . | Ref . |
---|---|---|---|
P(d) | |$8.66897\pm 0.00028$| | 1 | |
e | |$0.128\pm 0.028$| | 1 | |
HD 69830 b | K(m s−1) | |$3.4\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$10.1^{+0.38}_{-0.37}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.14^{+1.75}_{-0.34}$| | 2 | |
Orbital distance (AU) | |$0.079\pm 0.001$| | 2 | |
P(d) | |$31.6158\pm 0.0051$| | 1 | |
e | |$0.03\pm 0.03$| | 1 | |
HD 69830 c | K (m s−1) | |$2.6\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.09^{+0.55}_{-0.54}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.12}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.188\pm 0.001$| | 2 | |
P (d) | |$201.4\pm 0.4$| | 1 | |
e | |$0.08\pm 0.07$| | 1 | |
HD 69830 d | K (m s−1) | |$1.5\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.26^{+0.89}_{-0.88}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.17}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.644\pm 0.001$| | 2 |
Orbital parameter of exoplanets detected around HD 69830. The source of the values in the table (Ref) is given in the final column: 1.(Laliotis et al. 2023), 2. This study.
Planet . | Parameter . | Best fit . | Ref . |
---|---|---|---|
P(d) | |$8.66897\pm 0.00028$| | 1 | |
e | |$0.128\pm 0.028$| | 1 | |
HD 69830 b | K(m s−1) | |$3.4\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$10.1^{+0.38}_{-0.37}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.14^{+1.75}_{-0.34}$| | 2 | |
Orbital distance (AU) | |$0.079\pm 0.001$| | 2 | |
P(d) | |$31.6158\pm 0.0051$| | 1 | |
e | |$0.03\pm 0.03$| | 1 | |
HD 69830 c | K (m s−1) | |$2.6\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.09^{+0.55}_{-0.54}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.12}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.188\pm 0.001$| | 2 | |
P (d) | |$201.4\pm 0.4$| | 1 | |
e | |$0.08\pm 0.07$| | 1 | |
HD 69830 d | K (m s−1) | |$1.5\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.26^{+0.89}_{-0.88}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.17}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.644\pm 0.001$| | 2 |
Planet . | Parameter . | Best fit . | Ref . |
---|---|---|---|
P(d) | |$8.66897\pm 0.00028$| | 1 | |
e | |$0.128\pm 0.028$| | 1 | |
HD 69830 b | K(m s−1) | |$3.4\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$10.1^{+0.38}_{-0.37}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.14^{+1.75}_{-0.34}$| | 2 | |
Orbital distance (AU) | |$0.079\pm 0.001$| | 2 | |
P(d) | |$31.6158\pm 0.0051$| | 1 | |
e | |$0.03\pm 0.03$| | 1 | |
HD 69830 c | K (m s−1) | |$2.6\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.09^{+0.55}_{-0.54}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.12}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.188\pm 0.001$| | 2 | |
P (d) | |$201.4\pm 0.4$| | 1 | |
e | |$0.08\pm 0.07$| | 1 | |
HD 69830 d | K (m s−1) | |$1.5\pm 0.1$| | 1 |
M|$_{\rm P}$|sini (M|$_{\rm Earth}$|) | |$12.26^{+0.89}_{-0.88}$| | 1 | |
|$M_{\rm DA}$| (M|$_{\rm Jup}$|) | |$0.17^{+2.17}_{-0.11}$| | 2 | |
Orbital distance (AU) | |$0.644\pm 0.001$| | 2 |
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