J/AJ/170/153  CNEOS fireball light curves: BLADE classification  (Silber+, 2025)

BLADE: An automated framework for classifying light curves from the Center for Near-Earth Object Studies fireball database. Silber E.A., Sawal V. <Astron. J., 170, 153 (2025)> =2025AJ....170..153S 2025AJ....170..153S
ADC_Keywords: Photometry; Minor planets; Comets; Meteorites; Earth; Optical; Infrared; Models Keywords: Asteroids ; Meteoroids ; Light curves ; Light curve classification Abstract: Fireballs (bolides) are high-energy luminous phenomena produced when meteoroids and small asteroids enter Earth's atmosphere at hypersonic speeds, often resulting in fragmentation or complete disintegration accompanied by significant energy release. The resulting bolide light curves capture temporal brightness variations as these objects traverse increasingly dense atmospheric layers, providing essential information on meteoroid entry dynamics, fragmentation behavior, and atmospheric energy deposition processes. The Center for Near-Earth Object Studies' (CNEOS) continuously expanding fireball database offers a globally comprehensive archive of bolide events, including light curves and associated metadata. Events associated with infrasound detections allow direct correlations between acoustic signatures and light curve features, therefore enabling detailed analyses of fragmentation dynamics and energy deposition. Here, we introduce Bolide Light-curve Analysis and Discrimination Explorer (BLADE), a robust and high-fidelity framework specifically designed to analyze bolide light curves for objects detected from space. BLADE incorporates a processing pipeline integrating Savitzky-Golay filtering, prominence-based peak detection, and gradient analysis, enabling systematic identification and classification of fragmentation events and their associated energy release characteristics. Preliminary results demonstrate that BLADE reliably distinguishes distinct bolide behaviors, providing an objective, scalable methodology for characterization and analysis of large bolide light curve data sets. This foundational work establishes a novel pathway for advanced bolide research, with promising applications in planetary defense and global atmospheric monitoring. Future research should adopt an integrative approach combining CNEOS optical data with complementary infrasound measurements, further clarifying relationships between bolide energy deposition and acoustic signatures, thus refining our understanding of meteoroid and asteroid atmospheric entry processes. Description: At the time of this analysis, the Center for Near-Earth Object Studies' (CNEOS) fireball database, maintained by NASA's Jet Propulsion Laboratory (JPL), contained approximately 850 light curves documenting bolide events detected by U.S. Government (USG) sensors. The initial subset included 144 events, each having infrasound detections published in the literature. After careful evaluation of data quality and completeness in both optical and acoustic records, the final subset totaled 124 bolides. The light curve data were obtained directly from the CNEOS database (http://cneos.jpl.nasa.gov/fireballs/). Here, we use BLADE, an integrated framework comprising data preprocessing, Savitzky-Golay filtering for noise reduction, peak detection, gradient analysis, and event classification. The CNEOS fireball database is widely regarded as one of the most comprehensive observational archives available for studying meteoroid entry events and their interaction with Earth's atmosphere. Managed by NASA's JPL, the database aggregates observations from USG sensors, which detect bolides on a global scale through their radiative emissions in optical and infrared wavelengths. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 139 124 List of events and output classifications -------------------------------------------------------------------------------- See also: B/comets : Database of the orbital elements of comets (Rocher, 2007) J/AJ/156/60 : Thermal model fits for short-arc NEOs: NEOWISE (Masiero+, 2018) J/A+A/667/A157 : 824 fireballs observed in 2017-2018 (Borovicka+, 2022) J/A+A/679/A148 : Compositional properties of NEOs (Sergeyev+, 2023) J/A+A/674/A50 : Near-Earth Object (NEO) properties (Deshapriya+, 2023) J/A+A/682/A29 : Detection of the Yarkovsky effect on NEAs (Fenucci+, 2024) J/A+A/704/A241 : Calibrated spectra of 31 fireballs (Vojacek+, 2025) http://cneos.jpl.nasa.gov/fireballs/ : CNEOS fireball database (NASA JPL) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Event [147/905] CNEOS event number 5- 14 A10 "Y/M/D" Date Bolide event date 16- 23 A8 --- Time Bolide event time in UTC 25- 29 F5.1 deg Lat [-83.7/88.5] Bolide latitude 31- 36 F6.1 deg Long [-179.3/174.2] Bolide longitude 38- 41 F4.1 km Alt [16.7/59.3]? Bolide altitude 43- 46 F4.1 km/s Vel [9.8/44.8]? Velocity 48- 52 F5.1 km/s xVel [-35.4/21.3]? Velocity in x-direction 54- 58 F5.1 km/s yVel [-43.5/23.4]? Velocity in y-direction 60- 64 F5.1 km/s zVel [-31.2/23.9]? Velocity in z-direction 66- 73 E8.2 J Radiated [2.8/3.75e14] Total radiated energy 75- 81 F7.3 --- Impact [0.073/440.0] Total impact energy (1) 83- 88 F6.2 deg Azimuth [6.89/358.98]? Azimuth 90- 94 F5.2 deg Angle [4.42/83.54]? Entry angle 96- 119 A24 --- Type Fragmentation type (2) 121- 124 I4 yr Year [2000/2022] UTC year 126- 127 I2 month Month UTC month 129- 130 I2 d Day UTC day 132- 133 I2 h Hr UTC hour 135- 136 I2 min Min UTC minute 138- 139 I2 s Sec UTC second -------------------------------------------------------------------------------- Note (1): Expressed in units of kilotons (kt) of trinitrotoluene (TNT), where 1kt TNT = 4.184e12 J. Note (2): Fragmentation type as follows: Airburst = 9 occurrences Continuous Fragmentation = 3 occurrences Discrete Fragmentation = 81 occurrences Single Peak = 31 occurrences -------------------------------------------------------------------------------- History: From electronic version of the journal License: CC-BY-4.0
(End) Prepared by [AAS], Robin Leichtnam [CDS] 29-Jun-2026
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line