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Last updated: October 5, 2025

Comet Lemmon (C/2012 F6): The Southern Hemisphere's Green Visitor

Comet Lemmon with its characteristic green hue
Description: Comet Lemmon photographed from Siding Spring Observatory (Australia) on January 9, 2013. Its blue-green color (due to diatomic carbon C₂) and dust tail are clearly visible. Rolando Ligustri / Siding Spring Observatory.

An Extraordinary Comet

Comet Lemmon (C/2012 F6) captivated observers in 2012-2013 with its brilliant green color and exceptional visibility in the southern hemisphere. Discovered by the Mount Lemmon Survey in Arizona, it exemplifies the chemical and physical phenomena that define these icy travelers of the solar system.

What Is a Comet?

A comet is an icy celestial body composed of:

When a comet approaches the Sun (within 3-4 AU), the sublimation of ices creates:

Comet Lemmon (C/2012 F6) Fact Sheet
CharacteristicValue/Details
Official DesignationC/2012 F6 (Lemmon)
Discovery DateMarch 23, 2012 (Mount Lemmon Survey, Arizona, USA)
Orbit TypeHyperbolic (non-periodic)
Perihelion0.73 AU (March 24, 2013)
Peak Magnitude~5.5 (January 2013)
Distinctive ColorGreen (C₂ emission at 518 nm)
VisibilitySouthern Hemisphere (December 2012 - April 2013)
Minimum Distance to Earth0.98 AU (February 5, 2013)
DiscovererA.R. Gibbs
Notable CompositionDiatomic carbon (C₂), cyanogen (CN), silicate dust

N.B.:
Comets with hyperbolic orbits like Lemmon likely originate from the Oort Cloud and pass near the Sun only once before leaving the inner solar system permanently.

Why the Green Color?

The emerald hue of Comet Lemmon results from fluorescence:

  1. Solar ultraviolet radiation excites diatomic carbon (C₂) molecules in the coma.
  2. These molecules then emit light at 518 nm (green) when returning to their ground state.
  3. Cyanogen (CN) also contributes to this color (emission at 388 nm, violet).
Key Observation Timeline
DateEventMagnitudePosition
March 23, 2012Discovered by A.R. Gibbs20.8-
December 2012Visible with binoculars< 10Southern Hemisphere
January 9, 2013Peak visibility5.5Sagittarius
March 24, 2013Perihelion passage~60.73 AU from the Sun
April 2013Gradual disappearance> 10-

N.B.:
A magnitude of 5.5 is the naked-eye visibility limit under a perfectly dark sky. In cities, a magnitude of 4 or less is typically required for unaided observation.

How to Observe a Comet Like Lemmon?

Recommended Equipment:
Suitable Observation Equipment
Equipment TypeFeaturesPossible Observations
Naked EyeDark sky (limiting magnitude > 6)Fuzzy coma (no details)
Binoculars10×50 or 20×80Coma and short tail visible
Telescope≥ 150 mm apertureComa details, dust tail
PhotographyDSLR + long exposure (20-60 sec)Extended tails, colors (with processing)

N.B.:
Swan-Band or C₂ filters enhance gaseous structures in photography but reduce overall light by 30 to 50%.

Upcoming Passages of Comet Lemmon

Comet Lemmon (C/2012 F6) follows a hyperbolic trajectory, which means it will probably not return to the inner solar system regularly. A periodic comet (like Halley, Period ≈ 76 years) returns at predictable intervals. A hyperbolic comet has an open trajectory: it may pass near the Sun once or a few times, or escape permanently into interstellar space. In reality, the comet is moving away from the Sun and its path does not allow a "classic" orbital period to be defined.

Note :
Hyperbolic comets, unlike periodic comets, are not expected to have regular close passages. Any future observation would be exceptional and unpredictable on a human timescale.

Orbital Predictions for Comet Lemmon
YearMinimum Distance to the SunEstimated Distance from EarthRemarks
2012-20130.73 AU0.98 AUObserved from the Southern Hemisphere
2100 (simulation)~5 AU~4.8 AUDistant passage, not visible to the naked eye
20250.72 AU (close approach to the Sun)≈ 0.95 AUPossible naked-eye observation in the Southern Hemisphere

Note :
Hyperbolic comets, unlike periodic comets, do not have regular close passages. Any future observation would be exceptional and highly uncertain on a human timescale.

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