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Dear all, It is our pleasure to announce that we have completed our very first live event on Instagram. We were joined by fellow photographer Don Komarechka (@donkomphoto) to discuss the philosophical impact of macrophotography on Tuesday, 24 January 2023, at 7 PM Central European Time (1:00 PM Eastern Time / 10:00 AM Pacific Time). […]
Awe-inspiring images of
micrometeorites to remind you
that beauty truly is everywhere.
This season's collection features a variety of stunning micrometeorites. From mountainous cryptocrystalline turtlebacks and bewitching glass spherules to ultra rare giants. Available for a limited time only.
NMM 1448: V-TYPE
NMM 1448: V-TYPE
Glass or vitreous type (V-type) micrometeorites each a temperature of up to 2000°C (3600°F) as they descend through the atmosphere..
These delicate, translucent spherules are difficult to find due to their lack of magnetism, since most of their metals evaporated during descent.
NMM 1359: CC-TYPE
Cryptocrystalline (CC-type) micrometeorites are composed of glassy particles with fine-grained crystallites that are too small to recognize as individual grains.
Many of these magnificent spherules feature metal beads and aerodynamic forms, while others have a "turtleback" shape with humps distributed evenly around the spherule.
NMM 1359: CC-TYPE
NMM 1149: PO-TYPE
Porphyritic olivine (PO-type) micrometeorites are also made of forsterite, a type of olivine that is made of magnesium.
There are many morphological varieties of this type of micrometeorite; From evenly distributed small crystals, to crystals that increase in side, to extremely large or even possibly a single olivine crystal.
NMM 1149: PO-TYPE
NMM 1271: Sc-TYPE
When stardust does not reach a peak temperature of at least 1350°C (2500°F) during entry and deceleration, it barely melts. Volatile elements expand and escape in the form of gas bubbles, which results in a scoriaceous (SC-type) or vesicular micrometeorite.
Micrometeorites of this type are extremely difficult to find.
NMM 1271: SC-TYPE
NMM 1271: G-, I-, CAT-typeS
From G-types with dark silicate glass, I-types dominated by iron, and milky CAT spherules enriched with calcium, aluminum, and titanium, to fossil, unmelted, and un-categorized micrometeorites.
There is no question that Jon Larsen and Jan Braly Kihle's contributions have had a dramatic effect on the field.
NMM 1271: G-/I-/CAT-TYPES
From directors Werner Herzog and Clive Oppenheimer, this remarkable journey across our planet and universe explores how meteorites, shooting stars, and deep impacts have awoken our wonder about other realms-and make us rethink our destinies.
Never before has it been possible to see stardust in such a large format with crisp details. The 500+ color images are made possible by a new photo technology developed for this project by the author and mineralogist Jan Braly Kihle.
Jon Larsen revolutionized the study of micrometeorites when he became the first person to discover a micrometeorite from an urban environment. Then a new form of art emerged when he and Jan Braly Kihle created the world's first high resolution photographs of micrometeorites in colour.
Learn about the singular moment that led to Jon's groundbreaking discovery
and the phone call that kickstarted a truly epic friendship.
Jon Larsen revolutionized the study of micrometeorites when he became the first person to discover a micrometeorite from an urban environment. Then a new form of art emerged when he and Jan Braly Kihle created the world's first high resolution photographs of micrometeorites in colour.
Learn about the singular moment that led to Jon's groundbreaking discovery and the phone call that kickstarted a truly epic friendship.
I HAVE TO KNOW
I'm ready. TEACH ME.
Jon Larsen and Jan Braly Kihle have amassed the world's most expansive collection of urban micrometeorites and they want you to follow in their footsteps.