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Martian stick-like structures are not trace fossils: a new protocol for testing ichnogenicity synthesized from paleosol ichnology

Published online by Cambridge University Press:  03 September 2021

Jorge F. Genise*
Affiliation:
CONICET – Museo Argentino de Ciencias Naturales, División Icnología, Av. Ángel Gallardo 470, 1405 Buenos Aires, Argentina
*
Author for correspondence: Jorge F. Genise, E-mail: jgenise@macn.gov.ar
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Abstract

There are different criteria that are usually analysed independently before identifying a new trace fossil, such as morphological regularity, completeness, dispersion, recurrence and complexity, surface morphology, and context. The synthesis of these criteria, as utilized in paleosol ichnology, composes a protocol that is presented herein for the first time and can be used for testing the ichnogenicity of trace-like structures in any paleoenvironment of Earth or Mars. As a study case, the Martian ‘stick-like structures’ do not fulfil any of the requirements posed by this protocol to be postulated as trace fossils. The ichnogenicity test, focussed exclusively on morphology and context, is simpler but equally useful as the biogenicity ones. It may be applied in the future with other potential cases before carrying on more complex analyses or to evaluate the astrobiological interest of trace-like structures.

Information

Type
Research Article
Copyright
Copyright © The Author(s), 2021. Published by Cambridge University Press
Figure 0

Fig. 1. Stick-like structures from the Murray Formation at Vera Rubin Ridge in Gale Crater. Mars. Image 1923MH0007280000703207R00_DXXX from the Curiosity rover using MAHLI. Scale bar: 1 cm.

Figure 1

Fig. 2. Features of paleosol trace fossils and comparable structures. (A) Morphological regularity of some trace fossils from paleosols. (B) Completeness. Left column, on top an incomplete, truncated, specimen of Fictovichnus (chafer pupation chamber) that may be confused (below) with a specimen of Celliforma (bee cell). Right column, on top the external, little informative, aspect of a specimen of Coprinisphaera contrasting with its internal complex morphology (below). (C) Dispersion. On top, a collection of armoured clay nodules. Arrows indicate the most regular ones that may be confused with the trace fossil Rebuffoichnus. Below, a group of inorganic concretions, where arrows indicate two more regular spheroidal ones that may be confused with Coprinisphaera. (D) Complexity. Elipsoideichnus meyeri from the Eocene of Uruguay shows an extremely complex morphology. (E) Recurrence. A high concentration of Rebuffoichnus from the Pleistocene of Canary Islands. (F) Surface morphology. On the left a spheroidal concretion showing a smooth surface, on the right, a specimen of Pallisphaera puertai showing a pelletal surface morphology, both from the early Cretaceous of Argentina. All bar scales: 1 cm except for (E): 10 cm.

Figure 2

Fig. 3. Structures imaged on Mars compared to Earth trace fossils. (A) Linear structures (arrows) scattered on Mars surface at the Naukluft Plateau. Image 1278MH0001900010404672C00_DXXX from MAHLI of Curiosity rover. Scale bar: 1 cm. (B) Loose and broken rhizoliths (arrows) from the Oligocene Chilapa Formation of Mexico. Scale bar: 5 cm. (C) Cracked tubular structure (arrows) from the surface target ‘Pvt. Ebenezer Tuttle’ at Marathon Valley, Mars. Image 1M500516263EFFCONIP2935M2M1 from the MI of the Opportunity rover. Scale bar: 1 cm. (D) Cracked invertebrate burrow (arrows) from the Miocene Pinturas Formation of Argentina. Scale bar: 1 cm. (E) Structure showing a rounded and a flat extreme (arrow) from the surface target ‘Pvt. Ebenezer Tuttle’ at Marathon Valley, Mars. Image 1M500516482EFFCONIP2936M2M1 from the MI of the Opportunity rover. Scale bar: 5 mm. (F) Celliforma (arrow) from the Cretaceous Mercedes Formation of Uruguay. Scale bar: 1 cm. (G) Structure showing a bulbous end (right arrow) followed by an irregular cylinder (left arrow) from the surface target ‘Dibbler’ at Solander Point, Mars. Image 1M431365143EFFC7KDP2955M2M1 from the MI of the Opportunity rover. Scale bar: 5 mm. (H) Irregular tunnel (left arrow) ended in a specimen of Fictovichnus (right arrow) from the Miocene Calatayud-Daroca Basin of Spain. Scale bar: 1 cm.

Figure 3

Fig. 4. Three remains (arrows) vertically oriented, attached to one side of a step that is probably one side of a former crack observable below the fragments and more to the right and up below the stick-like structure. Image 1923MH0007280000703211R00_DXXX from the Curiosity rover using MAHLI. Scale bar: 1 cm.

Figure 4

Fig. 5. Panoramic views of neighbouring rocks of Haroldswick showing dark-toned, positive-relief features similar to stick-like structures. Images obtained by the Mastcam of the Curiosity rover during Sols 1905–1922. (A) Rocks near the stick-like structures (black arrow) showing from elongated to unshaped dark-toned structures, some of them showing sharp contacts with the rock. Only some of them are indicated with white arrows, and also a Y-V shaped form (yellow arrow). Image 1905MR0099940220900105E01_DXXX. (B) A rock about 20 m from Haroldswick showing dark-toned structures with unshaped to nodular structures (white arrow) and loose fragments in the surroundings. Image 1910ML0100170050704064E01_DXXX. (C) Several rocks about 15 m from Haroldswick showing a full relief dark-toned spot (yellow arrow) and several unshaped to V-shaped forms in the surroundings, some of them indicated with white arrows. Image 1910ML0100170040704063E01_DXXX. (D) A close up to the rock depicted in (C). Image 1911MR0100210000900178E01_DXXX. (E) A rock about 8 m from Haroldswick showing a straight to gently curved fracture fill preserved in full relief (white arrow). Image 1922ML0100350120704450E01_DXXX. (F) Close to (E) several dark-toned fracture fills preserved as full relief structures. Image 1922ML0100350130704451E01_DXXX.