2023ApJ...944L..35G


Query : 2023ApJ...944L..35G

2023ApJ...944L..35G - Astrophys. J., 944, L35 (2023/February-3)

A Second Earth-sized Planet in the Habitable Zone of the M Dwarf, TOI-700.

GILBERT E.A., VANDERBURG A., RODRIGUEZ J.E., HORD B.J., CLEMENT M.S., BARCLAY T., QUINTANA E.V., SCHLIEDER J.E., KANE S.R., JENKINS J.M., TWICKEN J.D., KUNIMOTO M., VANDERSPEK R., ARNEY G.N., CHARBONNEAU D., GUNTHER M.N., HUANG C.X., ISOPI G., KOSTOV V.B., KRISTIANSEN M.H., LATHAM D.W., MALLIA F., MAMAJEK E.E., MIRELES I., QUINN S.N., RICKER G.R., SCHULTE J., SEAGER S., SUISSA G., WINN J.N., YOUNGBLOOD A. and ZAPPARATA A.

Abstract (from CDS):

We report the discovery of TOI-700 e, a 0.95 R⊕ planet residing in the Optimistic Habitable Zone (HZ) of its host star. This discovery was enabled by multiple years of monitoring from NASA's Transiting Exoplanet Survey Satellite (TESS) mission. The host star, TOI-700 (TIC 150428135), is a nearby (31.1 pc), inactive, M2.5 dwarf (Vmag = 13.15). TOI-700 is already known to host three planets, including the small, HZ planet, TOI-700 d. The new planet has an orbital period of 27.8 days, and based on its radius (0.95 R⊕), it is likely rocky. TOI-700 was observed for 21 sectors over Years 1 and 3 of the TESS mission, including 10 sectors at 20 s cadence in Year 3. Using this full set of TESS data and additional follow-up observations, we identify, validate, and characterize TOI-700 e. This discovery adds another world to the short list of small, HZ planets transiting nearby and bright host stars. Such systems, where the stars are bright enough that follow-up observations are possible to constrain planet masses and atmospheres using current and future facilities, are incredibly valuable. The presence of multiple small, HZ planets makes this system even more enticing for follow-up observations.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Exoplanet systems - Transit photometry - Low-mass stars - M-dwarf stars - Astronomy data analysis

Simbad objects: 13

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Number of rows : 13
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 L 231-32 PM* 04 33 39.7200127728 -51 57 22.435373160     12.617 12.147   M3.0V 83 0
2 G 222-11 PM* 06 10 19.8468098360 +82 06 24.318574744   12.214   9.5   M2.5V 145 0
3 TOI-700 PM* 06 28 23.2285331376 -65 34 45.520447908   14.524 13.076 12.659 10.70 M2V 84 0
4 TOI-700d Pl 06 28 23.2285331376 -65 34 45.520447908           ~ 64 0
5 TOI-700e Pl 06 28 23.2285331376 -65 34 45.520447908           ~ 20 0
6 TOI-700c Pl 06 28 23.2285331376 -65 34 45.520447908           ~ 17 0
7 TOI-700b Pl 06 28 23.2285331376 -65 34 45.520447908           ~ 18 0
8 L 98-59 PM* 08 18 07.6214406393 -68 18 46.805365587   13.22 11.685 11.294 9.25 M3V 135 0
9 TOI-1749 PM* 18 50 57.0647942175 +64 25 09.119009331   15.126 13.809 13.352   ~ 23 0
10 Kepler-186 Er* 19 54 36.6535147488 +43 57 18.025920324   16.731 15.290 14.833   M1V 151 0
11 TRAPPIST-1 LM* 23 06 29.3684948589 -05 02 29.037301866     18.798 16.466 14.024 M7.5e 1306 0
12 TRAPPIST-1d Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 263 0
13 TRAPPIST-1c Pl 23 06 29.3684948589 -05 02 29.037301866           ~ 282 0

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