Lunar Reconnaissance Orbiter Camera

Cool Cold Spots

Einthoven cold spot crater oblique (side) view
Oblique (very!) view of Einthoven cold spot crater, located at 109.91° E, 6.74° S. White rays and the crater's rocky rim and rugged interior wall are visible signs of youth. The cold spot anomaly surrounding the crater is another sign of youth. It extends far beyond the three-kilometer width of this image, but is invisible to human eyes. NAC M1258299787L/R [NASA/GSFC/Arizona State University] 

The Lunar Reconnaissance Orbiter (LRO) spacecraft explores the Moon using seven scientific instruments. These include the LRO Camera (LROC) package, which is, of course, the instrument we highlight in these Featured Images. The seven instruments collect different kinds of scientific data. Combining their data sets allows scientists to make discoveries they never could if they were limited to a single lunar-orbiting instrument. 

Since 2009, the heat-sensing Diviner Lunar Radiometer Experiment on LRO has systematically mapped the Moon's surface temperatures, enabling reseachers to chart more than 2200 anomalous cold spots between 50° N and 50° S latitude. The cold spot anomalies appear after the Sun goes down.

The Diviner instrument sees the cold spots as irregular splotches that rapidly radiate heat after sunset until they are up to 10° Fahrenheit colder than the surrounding landscape. LROC, observing in the visible part of the spectrum, sees nothing unusual at cold spot locations. When the Sun rises, the spots rapidly warm to the temperature of their surroundings and blend in with the background.

On this map, colored dots mark the locations of cold spot craters. Blue dots are cold spot craters with diameters greater than 800 meters. The near-equatorial, farside blue dot labeled with the numeral 4 marks Einthoven cold spot crater. Image from Williams, et al (2018) [NASA/GSFC/UCLA]

What causes cold spot anomalies? In most cases, Diviner data are of too low a resolution to confirm a source. When Diviner data are overlaid on higher-resolution LROC images, however, researchers find that almost all occur around impact craters that are young (less than one million years) and small (from 43 meters to 2300 meters across).

We know the craters are young because they have very rocky floors and rims and are surrounded by bright rays. The steady infall of debris from space has not yet had time to chip away these signs of youth. This leads researchers to conclude that a process related to the formation of small craters creates the cold spot anomalies. But what process?

Einthoven cold spot crater, the subject of today's Featured Image, is 1143 m wide, or about the size of Meteor Crater in Arizona. So far, it has no official name — we call it Einthoven cold spot crater because it is just south of Einthoven crater, which is old, degraded, and, at 69 kilometers in diameter, the largest crater in the neighborhood.

Though craters associated with cold spot anomalies are small, the cold spots themselves are often large. The Einthoven cold spot crater anomaly takes in 2070 square kilometers of terrain and extends up to 50 kilometers from the crater.  That's much too large an area for ejecta from the crater to cover, which eliminates the most obvious cold spot formation hypothesis: that material blasted from the crater during its formation could create the cold spot. 

So, how to explain the cold spot anomalies? Some researchers invoke a cascading series of tiny secondary impacts traveling outward from the crater-forming asteroid impact, while others believe that gas produced by the impact flows through the top layer of lunar surface material. Either process might "fluff up" the surface, changing the way heat affects it. Few researchers, however, find these explanations to be 100% convincing.

Be sure to examine the Einthoven cold spot in the images below and follow the links to scientific papers about on-going efforts to solve the cold spot mystery!

In this oblique night-time view of Einthoven cold spot crater (center of image) and surrounding areas, the 1.1-kilometer-wide crater has a white floor because it is rocky and warm (rocks are good at absorbing and holding onto solar heat). Its rim and ejecta blanket, less rocky, are red and yellow, respectively. Dark blue marks the cold spot anomaly. The image is a section of an LROC WAC global mosaic draped over a Digital Elevation Model based on LRO Lunar Orbiting Laser Altimeter (LOLA) data and colorized with Diviner night-time surface temperature data. Image width is about 200 kilometers. [NASA/GSFC/UCLA]
The overhead night-time view above displays the extent of the Einthoven cold spot anomaly. The 1.1-kilometer crater is located near the center of the image.  The nearby crater Einthoven, for which the cold spot crater is informally named, is the largest crater in the image. Temperature range across the image is about 45° Fahrenheit, with white being warmest and dark blue coldest. This image, like the one above it, makes use of Diviner, LROC, and LOLA data sets. Image width about 200 kilometers. [NASA/GSFC/UCLA]

Related Featured Images

Ejecta Sweeps the Surface  Albedo contrast in the ejecta around a roughly one-kilometer-wide young crater in the Sea of Tranquility

Dynamic Textures  The ejecta blanket around a young 1.1-kilometer crater resembles a furrowed farm field

Ka-Pow! Complex ejecta patterns around a 650-meter young crater in 164-kilometerJoliot crater

Minty Fresh A 330-meter young farside crater with complex rays

Dynamic Moon! LROC reached the Moon in 2009 — by imaging the same places repeatedly over the years and comparing the images we've discovered many new small craters and dark "splotches"

Scientific Papers on Lunar Cold Spots

Mendell, W. W., and Low, F. J. (1975), "Infrared Orbital Mapping of Lunar Features,"  Proc. Lunar Sci. Conf. 6th, 2711-2719 https://www.researchgate.net/publication/23924054/download

Bandfield, J. L., Ghent, R. R., Vasavada, A. R., Paige, D. A., Lawrence, S. J., Robinson, M. S. (2011), "Lunar Rock Abundance and Regolith Fines Derived From LRO Diviner Radiometer Data," Journal of Geophysical Research, 116, E00H02 https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2011JE003866

Bandfield, J. L,, Song, E., Hayne, P. O., Brand, B. D., Ghent, R. R., Vasavada, A. R., Paige, D. A. (2014), "Lunar Cold Spots: Granular Flow Features and Extensive Insulating Materials Surrounding Young Craters," Icarus, 231, 221-231 https://pdfs.semanticscholar.org/49fb/c505b271f4dd57c5b30eaa4e4c9722ec2111.pdf?_ga=2.86897880.1912966133.1534358829-923306937.1534358829

Williams, J.-P., Paige, D. A., Greenhagen, B. T., Sefton-Nash, E. (2017), "The Global Surface Temperatures of the Moon as Measured by the Diviner Lunar Radiometer Experiment," Icarus, 283, 300-325 https://www.sciencedirect.com/science/article/pii/S0019103516304869

Williams, J.-P., Bandfield, J. L., Paige, D. A., Powell, T., Greenhagen, B. T., Taylor, S., Hayne, P. O., Speyerer, E. J., Ghent, R. R., Costello, E. S. (2018), "Lunar Cold Spots and Crater Production on Moon," Journal of Geophysical Research, in press http://adsabs.harvard.edu/abs/2016DPS....4821505W


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