Dr. Felisa Smith | Smith Lab

Bio:
Felisa Smith is a Distinguished Professor in the department of Biology. A conservation paleoecologist, she integrates modern, historic and fossil mammal records to investigate pressing environmental issues such as climate change and biodiversity loss. Over her career she has worked on organisms from microbes to mammoth, but vastly prefers the latter. Most recently Smith has been using the terminal Pleistocene megafauna extinction as a proxy for understanding modern mammal biodiversity loss. In addition to her 3 books, she has written~120 papers/book chapters in a wide variety of scientific journals, and taught scientific blogging at UNM (http://unm-bioblog.blogspot.com). She has participated in many audio and video programs including National Public Radio, BBC World Service, BBC Earth, and BBC’s Horizon series, German public radio, the Canadian Broadcasting Corporation, and the History Channel as well as numerous print interviews/essays. Felisa was elected a Fellow of the Paleontological Society in 2020, was awarded the Merriam Award from the American Society of Mammalogists in 2022, and is the 68th recipient of the UM Annual Research Lecturership in 2023. She is currently the President of the American Society of Mammalogists and Past President of the International Biogeography Society.

Abstract:
The conservation status of large-bodied mammals is dire. Their decline has serious consequences because they have unique ecological roles not replicated by smaller-bodied animals. Here, we use the fossil record of the megafauna extinction at the terminal Pleistocene to explore the consequences of past biodiversity loss. We characterize the isotopic and body-size niche of a mammal community in Texas before and after the event to assess the influence on the ecology and ecological interactions of surviving species (>1kg). Pre-extinction, a variety of C₄-grazers, C₃-browsers, and mixed-feeders existed, similar to modern African savannas, with likely specialization among the two sabertooth cats for juvenile grazers. Post-extinction, body size and isotopic niche space were lost, and the δ¹³C and δ¹⁵N values of some survivors shifted. We see mesocarnivore release within the Felidae: the jaguar, now an apex carnivore, moved into the specialized isotopic niche previously occupied by extinct cats. Puma, previously absent, became common and lynx shifted towards consuming more C₄-based resources. Lagomorphs were the only herbivores to shift towards C₄ resources. Body size changes from the Pleistocene to Holocene were species-specific, with some animals (deer, hare) becoming significantly larger, and others smaller (bison, rabbits) or exhibiting no change to climate shifts or biodiversity loss. Overall, the Holocene body size-isotopic niche was drastically reduced and considerable ecological complexity lost. We conclude biodiversity loss led to reorganization of survivors and many ‘missing pieces’ within our community; without intervention, the loss of Earth’s remaining ecosystems that support megafauna will likely suffer the same fate.

Dr. Smith at Texas Memorial Museum

Fossils under study

Cave art showing human hunting

Dr. Felisa Smith | Smith Lab

Bio:
Felisa Smith is a Distinguished Professor in the department of Biology. A conservation paleoecologist, she integrates modern, historic and fossil mammal records to investigate pressing environmental issues such as climate change and biodiversity loss. Over her career she has worked on organisms from microbes to mammoth, but vastly prefers the latter. Most recently Smith has been using the terminal Pleistocene megafauna extinction as a proxy for understanding modern mammal biodiversity loss. In addition to her 3 books, she has written~120 papers/book chapters in a wide variety of scientific journals, and taught scientific blogging at UNM (http://unm-bioblog.blogspot.com). She has participated in many audio and video programs including National Public Radio, BBC World Service, BBC Earth, and BBC’s Horizon series, German public radio, the Canadian Broadcasting Corporation, and the History Channel as well as numerous print interviews/essays. Felisa was elected a Fellow of the Paleontological Society in 2020, was awarded the Merriam Award from the American Society of Mammalogists in 2022, and is the 68th recipient of the UM Annual Research Lecturership in 2023. She is currently the President of the American Society of Mammalogists and Past President of the International Biogeography Society.

Abstract:
The conservation status of large-bodied mammals is dire. Their decline has serious consequences because they have unique ecological roles not replicated by smaller-bodied animals. Here, we use the fossil record of the megafauna extinction at the terminal Pleistocene to explore the consequences of past biodiversity loss. We characterize the isotopic and body-size niche of a mammal community in Texas before and after the event to assess the influence on the ecology and ecological interactions of surviving species (>1kg). Pre-extinction, a variety of C₄-grazers, C₃-browsers, and mixed-feeders existed, similar to modern African savannas, with likely specialization among the two sabertooth cats for juvenile grazers. Post-extinction, body size and isotopic niche space were lost, and the δ¹³C and δ¹⁵N values of some survivors shifted. We see mesocarnivore release within the Felidae: the jaguar, now an apex carnivore, moved into the specialized isotopic niche previously occupied by extinct cats. Puma, previously absent, became common and lynx shifted towards consuming more C₄-based resources. Lagomorphs were the only herbivores to shift towards C₄ resources. Body size changes from the Pleistocene to Holocene were species-specific, with some animals (deer, hare) becoming significantly larger, and others smaller (bison, rabbits) or exhibiting no change to climate shifts or biodiversity loss. Overall, the Holocene body size-isotopic niche was drastically reduced and considerable ecological complexity lost. We conclude biodiversity loss led to reorganization of survivors and many ‘missing pieces’ within our community; without intervention, the loss of Earth’s remaining ecosystems that support megafauna will likely suffer the same fate.

Dr. Smith at Texas Memorial Museum

Fossils under study

Cave art showing human hunting

Dr. Felisa Smith | Smith Lab

Bio:
Felisa Smith is a Distinguished Professor in the department of Biology. A conservation paleoecologist, she integrates modern, historic and fossil mammal records to investigate pressing environmental issues such as climate change and biodiversity loss. Over her career she has worked on organisms from microbes to mammoth, but vastly prefers the latter. Most recently Smith has been using the terminal Pleistocene megafauna extinction as a proxy for understanding modern mammal biodiversity loss. In addition to her 3 books, she has written~120 papers/book chapters in a wide variety of scientific journals, and taught scientific blogging at UNM (http://unm-bioblog.blogspot.com). She has participated in many audio and video programs including National Public Radio, BBC World Service, BBC Earth, and BBC’s Horizon series, German public radio, the Canadian Broadcasting Corporation, and the History Channel as well as numerous print interviews/essays. Felisa was elected a Fellow of the Paleontological Society in 2020, was awarded the Merriam Award from the American Society of Mammalogists in 2022, and is the 68th recipient of the UM Annual Research Lecturership in 2023. She is currently the President of the American Society of Mammalogists and Past President of the International Biogeography Society.

Abstract:
The conservation status of large-bodied mammals is dire. Their decline has serious consequences because they have unique ecological roles not replicated by smaller-bodied animals. Here, we use the fossil record of the megafauna extinction at the terminal Pleistocene to explore the consequences of past biodiversity loss. We characterize the isotopic and body-size niche of a mammal community in Texas before and after the event to assess the influence on the ecology and ecological interactions of surviving species (>1kg). Pre-extinction, a variety of C₄-grazers, C₃-browsers, and mixed-feeders existed, similar to modern African savannas, with likely specialization among the two sabertooth cats for juvenile grazers. Post-extinction, body size and isotopic niche space were lost, and the δ¹³C and δ¹⁵N values of some survivors shifted. We see mesocarnivore release within the Felidae: the jaguar, now an apex carnivore, moved into the specialized isotopic niche previously occupied by extinct cats. Puma, previously absent, became common and lynx shifted towards consuming more C₄-based resources. Lagomorphs were the only herbivores to shift towards C₄ resources. Body size changes from the Pleistocene to Holocene were species-specific, with some animals (deer, hare) becoming significantly larger, and others smaller (bison, rabbits) or exhibiting no change to climate shifts or biodiversity loss. Overall, the Holocene body size-isotopic niche was drastically reduced and considerable ecological complexity lost. We conclude biodiversity loss led to reorganization of survivors and many ‘missing pieces’ within our community; without intervention, the loss of Earth’s remaining ecosystems that support megafauna will likely suffer the same fate.

Dr. Smith at Texas Memorial Museum

Fossils under study

Cave art showing human hunting

Dr. Felisa Smith | Smith Lab

Bio:
Felisa Smith is a Distinguished Professor in the department of Biology. A conservation paleoecologist, she integrates modern, historic and fossil mammal records to investigate pressing environmental issues such as climate change and biodiversity loss. Over her career she has worked on organisms from microbes to mammoth, but vastly prefers the latter. Most recently Smith has been using the terminal Pleistocene megafauna extinction as a proxy for understanding modern mammal biodiversity loss. In addition to her 3 books, she has written~120 papers/book chapters in a wide variety of scientific journals, and taught scientific blogging at UNM (http://unm-bioblog.blogspot.com). She has participated in many audio and video programs including National Public Radio, BBC World Service, BBC Earth, and BBC’s Horizon series, German public radio, the Canadian Broadcasting Corporation, and the History Channel as well as numerous print interviews/essays. Felisa was elected a Fellow of the Paleontological Society in 2020, was awarded the Merriam Award from the American Society of Mammalogists in 2022, and is the 68th recipient of the UM Annual Research Lecturership in 2023. She is currently the President of the American Society of Mammalogists and Past President of the International Biogeography Society.

Abstract:
The conservation status of large-bodied mammals is dire. Their decline has serious consequences because they have unique ecological roles not replicated by smaller-bodied animals. Here, we use the fossil record of the megafauna extinction at the terminal Pleistocene to explore the consequences of past biodiversity loss. We characterize the isotopic and body-size niche of a mammal community in Texas before and after the event to assess the influence on the ecology and ecological interactions of surviving species (>1kg). Pre-extinction, a variety of C₄-grazers, C₃-browsers, and mixed-feeders existed, similar to modern African savannas, with likely specialization among the two sabertooth cats for juvenile grazers. Post-extinction, body size and isotopic niche space were lost, and the δ¹³C and δ¹⁵N values of some survivors shifted. We see mesocarnivore release within the Felidae: the jaguar, now an apex carnivore, moved into the specialized isotopic niche previously occupied by extinct cats. Puma, previously absent, became common and lynx shifted towards consuming more C₄-based resources. Lagomorphs were the only herbivores to shift towards C₄ resources. Body size changes from the Pleistocene to Holocene were species-specific, with some animals (deer, hare) becoming significantly larger, and others smaller (bison, rabbits) or exhibiting no change to climate shifts or biodiversity loss. Overall, the Holocene body size-isotopic niche was drastically reduced and considerable ecological complexity lost. We conclude biodiversity loss led to reorganization of survivors and many ‘missing pieces’ within our community; without intervention, the loss of Earth’s remaining ecosystems that support megafauna will likely suffer the same fate.

Dr. Smith at Texas Memorial Museum

Fossils under study

Cave art showing human hunting

Dr. Felisa Smith | Smith Lab

Bio:
Felisa Smith is a Distinguished Professor in the department of Biology. A conservation paleoecologist, she integrates modern, historic and fossil mammal records to investigate pressing environmental issues such as climate change and biodiversity loss. Over her career she has worked on organisms from microbes to mammoth, but vastly prefers the latter. Most recently Smith has been using the terminal Pleistocene megafauna extinction as a proxy for understanding modern mammal biodiversity loss. In addition to her 3 books, she has written~120 papers/book chapters in a wide variety of scientific journals, and taught scientific blogging at UNM (http://unm-bioblog.blogspot.com). She has participated in many audio and video programs including National Public Radio, BBC World Service, BBC Earth, and BBC’s Horizon series, German public radio, the Canadian Broadcasting Corporation, and the History Channel as well as numerous print interviews/essays. Felisa was elected a Fellow of the Paleontological Society in 2020, was awarded the Merriam Award from the American Society of Mammalogists in 2022, and is the 68th recipient of the UM Annual Research Lecturership in 2023. She is currently the President of the American Society of Mammalogists and Past President of the International Biogeography Society.

Abstract:
The conservation status of large-bodied mammals is dire. Their decline has serious consequences because they have unique ecological roles not replicated by smaller-bodied animals. Here, we use the fossil record of the megafauna extinction at the terminal Pleistocene to explore the consequences of past biodiversity loss. We characterize the isotopic and body-size niche of a mammal community in Texas before and after the event to assess the influence on the ecology and ecological interactions of surviving species (>1kg). Pre-extinction, a variety of C₄-grazers, C₃-browsers, and mixed-feeders existed, similar to modern African savannas, with likely specialization among the two sabertooth cats for juvenile grazers. Post-extinction, body size and isotopic niche space were lost, and the δ¹³C and δ¹⁵N values of some survivors shifted. We see mesocarnivore release within the Felidae: the jaguar, now an apex carnivore, moved into the specialized isotopic niche previously occupied by extinct cats. Puma, previously absent, became common and lynx shifted towards consuming more C₄-based resources. Lagomorphs were the only herbivores to shift towards C₄ resources. Body size changes from the Pleistocene to Holocene were species-specific, with some animals (deer, hare) becoming significantly larger, and others smaller (bison, rabbits) or exhibiting no change to climate shifts or biodiversity loss. Overall, the Holocene body size-isotopic niche was drastically reduced and considerable ecological complexity lost. We conclude biodiversity loss led to reorganization of survivors and many ‘missing pieces’ within our community; without intervention, the loss of Earth’s remaining ecosystems that support megafauna will likely suffer the same fate.

Dr. Smith at Texas Memorial Museum

Fossils under study

Cave art showing human hunting

Dr. Antonio Lazcano Araujo 

Bio:
Antonio Lazcano is Distinguished Professor at the Universidad Nacional Autónoma de México, where he works on the origin and early evolution of life. He has worked in prebiotic chemistry, analyses of meteorites and, more lately, on bioinformatics and the reconstruction of early stages of celular evolution. He is author or coauthor of about 200 research papers and chapters in books. He has written several boioks for the general public, including El Origen de la Vida, La Chispa de la Vida y La Bacteria Prodigiosa. He has been Visiting Professor or Scholar in Residence at the Univeristy of Habana, Autónoma de Madrid, Houston, Valencia, Orsay Paris-Sud, University of California, San Diego, Universita di Roma La Sapienza, Institut Pasteur, ETH Zentrum in Zurich and the A. N. Bakh Institute of Biochemistry of the USSR. For ten years he was part of the NASA Astrobiology Institute Oversee Committee, and President of the Gordon Research Conference of the Origins of Life, and twice President of the International Society for the Study of the Origins of Life, being so far the only Latin American scientist to hold this position. He has received three Honoris causa, one from the Universita di Milano (Italy, 2008), one from the Universidad de Valencia (Spain, 2014), and a third one in 2015 from the  Universidad de Michoacan (Mexico). In 2013 the Third World Summit of Evolution granted him the Charles Darwin Distinguished Scientist Award, and in 2018 the College de France granted him the Guillaume Bude Medal. In October 2014 he was elected to the Colegio Nacional, the most Mexican important academic and cultural institution.

Abstract:
Led by Oparin’s hypothesis on a heterotrophic origin of life, in the early 1950s Stanley L. Miller began his PhD thesis under the supervision of Harold C. Urey, attempting to simulate the conditions of the primitive Earth. To do this, Miller placed a mixture of methane, ammonia, and hydrogen in a flask, to which water vapor from another flask simulating the primitive seas of the planet was added. After subjecting the mixture of gases to the action of electrical discharges, Miller found that in a very short time amino acids, urea, and other compounds of biochemical importance had been formed. The experiment was considered a demonstration of the premises of Oparin's theory, and marks the origin of the experimental study of the appearance of life. Analyses of the original samples from Miller's experiment using contemporary techniques has shown that the variety of compounds formed abiotically is much greater than originally reported, allowing a more complete picture of the processes that led to the origin of the first organisms.

Watch the seminar here!

Dr. Antonio Lazcano Araujo 

Bio:
Antonio Lazcano is Distinguished Professor at the Universidad Nacional Autónoma de México, where he works on the origin and early evolution of life. He has worked in prebiotic chemistry, analyses of meteorites and, more lately, on bioinformatics and the reconstruction of early stages of celular evolution. He is author or coauthor of about 200 research papers and chapters in books. He has written several boioks for the general public, including El Origen de la Vida, La Chispa de la Vida y La Bacteria Prodigiosa. He has been Visiting Professor or Scholar in Residence at the Univeristy of Habana, Autónoma de Madrid, Houston, Valencia, Orsay Paris-Sud, University of California, San Diego, Universita di Roma La Sapienza, Institut Pasteur, ETH Zentrum in Zurich and the A. N. Bakh Institute of Biochemistry of the USSR. For ten years he was part of the NASA Astrobiology Institute Oversee Committee, and President of the Gordon Research Conference of the Origins of Life, and twice President of the International Society for the Study of the Origins of Life, being so far the only Latin American scientist to hold this position. He has received three Honoris causa, one from the Universita di Milano (Italy, 2008), one from the Universidad de Valencia (Spain, 2014), and a third one in 2015 from the  Universidad de Michoacan (Mexico). In 2013 the Third World Summit of Evolution granted him the Charles Darwin Distinguished Scientist Award, and in 2018 the College de France granted him the Guillaume Bude Medal. In October 2014 he was elected to the Colegio Nacional, the most Mexican important academic and cultural institution.

Abstract:
Led by Oparin’s hypothesis on a heterotrophic origin of life, in the early 1950s Stanley L. Miller began his PhD thesis under the supervision of Harold C. Urey, attempting to simulate the conditions of the primitive Earth. To do this, Miller placed a mixture of methane, ammonia, and hydrogen in a flask, to which water vapor from another flask simulating the primitive seas of the planet was added. After subjecting the mixture of gases to the action of electrical discharges, Miller found that in a very short time amino acids, urea, and other compounds of biochemical importance had been formed. The experiment was considered a demonstration of the premises of Oparin's theory, and marks the origin of the experimental study of the appearance of life. Analyses of the original samples from Miller's experiment using contemporary techniques has shown that the variety of compounds formed abiotically is much greater than originally reported, allowing a more complete picture of the processes that led to the origin of the first organisms.

Watch the seminar here!

Dr. Antonio Lazcano Araujo 

Bio:
Antonio Lazcano is Distinguished Professor at the Universidad Nacional Autónoma de México, where he works on the origin and early evolution of life. He has worked in prebiotic chemistry, analyses of meteorites and, more lately, on bioinformatics and the reconstruction of early stages of celular evolution. He is author or coauthor of about 200 research papers and chapters in books. He has written several boioks for the general public, including El Origen de la Vida, La Chispa de la Vida y La Bacteria Prodigiosa. He has been Visiting Professor or Scholar in Residence at the Univeristy of Habana, Autónoma de Madrid, Houston, Valencia, Orsay Paris-Sud, University of California, San Diego, Universita di Roma La Sapienza, Institut Pasteur, ETH Zentrum in Zurich and the A. N. Bakh Institute of Biochemistry of the USSR. For ten years he was part of the NASA Astrobiology Institute Oversee Committee, and President of the Gordon Research Conference of the Origins of Life, and twice President of the International Society for the Study of the Origins of Life, being so far the only Latin American scientist to hold this position. He has received three Honoris causa, one from the Universita di Milano (Italy, 2008), one from the Universidad de Valencia (Spain, 2014), and a third one in 2015 from the  Universidad de Michoacan (Mexico). In 2013 the Third World Summit of Evolution granted him the Charles Darwin Distinguished Scientist Award, and in 2018 the College de France granted him the Guillaume Bude Medal. In October 2014 he was elected to the Colegio Nacional, the most Mexican important academic and cultural institution.

Abstract:
Led by Oparin’s hypothesis on a heterotrophic origin of life, in the early 1950s Stanley L. Miller began his PhD thesis under the supervision of Harold C. Urey, attempting to simulate the conditions of the primitive Earth. To do this, Miller placed a mixture of methane, ammonia, and hydrogen in a flask, to which water vapor from another flask simulating the primitive seas of the planet was added. After subjecting the mixture of gases to the action of electrical discharges, Miller found that in a very short time amino acids, urea, and other compounds of biochemical importance had been formed. The experiment was considered a demonstration of the premises of Oparin's theory, and marks the origin of the experimental study of the appearance of life. Analyses of the original samples from Miller's experiment using contemporary techniques has shown that the variety of compounds formed abiotically is much greater than originally reported, allowing a more complete picture of the processes that led to the origin of the first organisms.

Watch the seminar here!

Dr. Antonio Lazcano Araujo 

Bio:
Antonio Lazcano is Distinguished Professor at the Universidad Nacional Autónoma de México, where he works on the origin and early evolution of life. He has worked in prebiotic chemistry, analyses of meteorites and, more lately, on bioinformatics and the reconstruction of early stages of celular evolution. He is author or coauthor of about 200 research papers and chapters in books. He has written several boioks for the general public, including El Origen de la Vida, La Chispa de la Vida y La Bacteria Prodigiosa. He has been Visiting Professor or Scholar in Residence at the Univeristy of Habana, Autónoma de Madrid, Houston, Valencia, Orsay Paris-Sud, University of California, San Diego, Universita di Roma La Sapienza, Institut Pasteur, ETH Zentrum in Zurich and the A. N. Bakh Institute of Biochemistry of the USSR. For ten years he was part of the NASA Astrobiology Institute Oversee Committee, and President of the Gordon Research Conference of the Origins of Life, and twice President of the International Society for the Study of the Origins of Life, being so far the only Latin American scientist to hold this position. He has received three Honoris causa, one from the Universita di Milano (Italy, 2008), one from the Universidad de Valencia (Spain, 2014), and a third one in 2015 from the  Universidad de Michoacan (Mexico). In 2013 the Third World Summit of Evolution granted him the Charles Darwin Distinguished Scientist Award, and in 2018 the College de France granted him the Guillaume Bude Medal. In October 2014 he was elected to the Colegio Nacional, the most Mexican important academic and cultural institution.

Abstract:
Led by Oparin’s hypothesis on a heterotrophic origin of life, in the early 1950s Stanley L. Miller began his PhD thesis under the supervision of Harold C. Urey, attempting to simulate the conditions of the primitive Earth. To do this, Miller placed a mixture of methane, ammonia, and hydrogen in a flask, to which water vapor from another flask simulating the primitive seas of the planet was added. After subjecting the mixture of gases to the action of electrical discharges, Miller found that in a very short time amino acids, urea, and other compounds of biochemical importance had been formed. The experiment was considered a demonstration of the premises of Oparin's theory, and marks the origin of the experimental study of the appearance of life. Analyses of the original samples from Miller's experiment using contemporary techniques has shown that the variety of compounds formed abiotically is much greater than originally reported, allowing a more complete picture of the processes that led to the origin of the first organisms.

Watch the seminar here!

Dr. Antonio Lazcano Araujo 

Bio:
Antonio Lazcano is Distinguished Professor at the Universidad Nacional Autónoma de México, where he works on the origin and early evolution of life. He has worked in prebiotic chemistry, analyses of meteorites and, more lately, on bioinformatics and the reconstruction of early stages of celular evolution. He is author or coauthor of about 200 research papers and chapters in books. He has written several boioks for the general public, including El Origen de la Vida, La Chispa de la Vida y La Bacteria Prodigiosa. He has been Visiting Professor or Scholar in Residence at the Univeristy of Habana, Autónoma de Madrid, Houston, Valencia, Orsay Paris-Sud, University of California, San Diego, Universita di Roma La Sapienza, Institut Pasteur, ETH Zentrum in Zurich and the A. N. Bakh Institute of Biochemistry of the USSR. For ten years he was part of the NASA Astrobiology Institute Oversee Committee, and President of the Gordon Research Conference of the Origins of Life, and twice President of the International Society for the Study of the Origins of Life, being so far the only Latin American scientist to hold this position. He has received three Honoris causa, one from the Universita di Milano (Italy, 2008), one from the Universidad de Valencia (Spain, 2014), and a third one in 2015 from the  Universidad de Michoacan (Mexico). In 2013 the Third World Summit of Evolution granted him the Charles Darwin Distinguished Scientist Award, and in 2018 the College de France granted him the Guillaume Bude Medal. In October 2014 he was elected to the Colegio Nacional, the most Mexican important academic and cultural institution.

Abstract:
Led by Oparin’s hypothesis on a heterotrophic origin of life, in the early 1950s Stanley L. Miller began his PhD thesis under the supervision of Harold C. Urey, attempting to simulate the conditions of the primitive Earth. To do this, Miller placed a mixture of methane, ammonia, and hydrogen in a flask, to which water vapor from another flask simulating the primitive seas of the planet was added. After subjecting the mixture of gases to the action of electrical discharges, Miller found that in a very short time amino acids, urea, and other compounds of biochemical importance had been formed. The experiment was considered a demonstration of the premises of Oparin's theory, and marks the origin of the experimental study of the appearance of life. Analyses of the original samples from Miller's experiment using contemporary techniques has shown that the variety of compounds formed abiotically is much greater than originally reported, allowing a more complete picture of the processes that led to the origin of the first organisms.

Watch the seminar here!