Home » Tech » Comet 3I/Atlas: Orbital Period Shocks Scientists

Comet 3I/Atlas: Orbital Period Shocks Scientists

by Lisa Park - Tech Editor

Here’s a breakdown of the key findings ⁤and information from the provided text, categorized for clarity:

1. Comet Identification‌ &⁣ Observation Details:

* Comet name: 3I/ATLAS
* Origin: Interstellar ⁣(though properties suggest origin ​in the ​outer Solar System)
* Finding: Shortly before closest approach ⁣to Earth.
* Closest Approach to Earth: December 19th, at 273 million kilometers.
* Telescopes Used:

* Southern African​ Large Telescope
* Nordic Optical Telescope
* Calibration: Data calibrated using field stars from the ATLAS ‍and Apass catalogs.

2. Physical Characteristics & Activity:

* Rotation period: ​ 16.16 ± 0.01 hours
*‌ ​ Light Curve Amplitude: Approximately 0.3 magnitudes
* Dust Activity: Increased during​ the ‍observation period.
* Color: Colorful redness​ observed.
*‌ ⁤ Tail: No visible tail detected ⁣(likely‍ due to‌ observation geometry and​ low ⁢dust production).
* ​ Dust Production: Low.
* ⁤ Powder Mass ⁣Loss Rate: 0.3 – 4.2 kg/s (consistent with weakly active comets from the outer Solar System).
* Spectral Colors: Similar to​ comets in the outer Solar System, different from ⁤previous reports for 3I/ATLAS.

3. Key Findings &​ Conclusions:

* The comet’s properties ⁢(morphological and photometric) are consistent with a weakly active comet originating in the⁤ outer Solar System, despite its interstellar origin.
* Continued⁤ monitoring‍ around perihelion (closest⁤ approach to the Sun)⁣ is recommended to track changes in activity and color. This will provide valuable information about the evolution of interstellar materials under solar⁣ radiation.

4. Critically importent Terms Highlighted ⁢in ‍the Text:

* ​ ATLAS & Apass: Catalogs used​ for calibration.
* ⁤ Rotation Period: The time ⁤it takes for the‍ comet to complete one rotation.
* Southern African Large Telescope & Nordic Optical Telescope: Observatories ⁣used for data collection.
* Light Curve Amplitude: A measure⁢ of the variation in brightness as the comet ‌rotates.
* Increased Dust Activity: ⁣More dust being released from the comet.
* Colorful Redness: The comet’s color.
* Observation Geometry: ​The⁢ position ⁣of the Earth, Sun, and comet relative to each other.
*​ Low dust Production: A small amount of dust‍ being ​released.
*⁢ Powder Mass Loss Rates: The rate at which dust is being lost from the comet.
* ⁤ Spectral Colors: The distribution of colors in the comet’s light.
* morphological and photometric: Relating ‍to the shape and brightness of‍ the comet.
* Weakly active comet of origin in the outer Solar System: A comet‌ that is not ⁢very active and likely originated far from ‌the ⁤Sun.
* ⁤ Closest approach to Earth: The point ⁤in the comet’s orbit when it is ⁣nearest to Earth.

You may also like

Leave a Comment

This site uses Akismet to reduce spam. Learn how your comment data is processed.