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Table 5

Comparative table of Delorme 1 b’s disk and disks around more massive objects observed with MIRI/MRS.

Properties Delorme 1 AB b J0438 J0446B Typical Typical
Host type Exoplanet Brown dwarf VLMS T Tauri VLMS/BD
Age (Myrs) 30 ~0.6 34 1-10 1-10
Spectral Type L0 M7.25 M4.5 K0-M5 M4.5-M9
Distance (pc) 47.2 140.3 82
M* (M) 0.013 0.05 0.18 ~0.2-2 ~0.02-0.2
L* (L) 0.0003 0.002 0.016 ~0.01-0.2 ~0.1-0.002
(M/yr) 0.2-5×10−11 a 1.58×10−11 2.5×10−11 10−7-10−9 10−9-10−12
Lacc/L* 1-37% 4% 2.5% 1-100% 0.1-10%

Molecular emission

H2O b b
CO2
OH
HCN
CH4
CH3
C2H2
13CCH2
C2H4
C3H4
C4H2
C6H6
C2H6
HC3n
H2
References This work 1 2 3, 4 4, 5

Notes. aValues based on stellar and planetary scaling from Betti et al. (2022). bMarginal or weak detections. References. (1) Long et al. (2025), (2) Perotti et al. (2025), (3) Pascucci et al. (2023) for the typical values, (4) Grant et al. (2025); Arabhavi et al. (2025a) for the molecules detected in averaged MIR spectra, (5) Typical VLMS and BD properties comes from the sample describe in Arabhavi et al. (2025a), and references therein. These targets are selected for their similar properties, such as accretion rate, detected molecules, and age (e.g., J0446B), or for their proximity in mass (e.g., J0438), along with averaged values of T Tauri stars and VLMS observed at MIR (Grant et al. 2025; Arabhavi et al. 2025a).

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