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Pasadena police shoot and kill man after he crashes into Tesla, video footage reveals

A tragic incident unfolded in Pasadena on Saturday night when a 36-year-old man, identified as Ricardo Guade Andrade of San Fernando, was fatally shot by police after fleeing from officers and crashing into a parked Tesla. The chain of events began when officers discovered a parked white pickup truck facing the wrong direction on a one-way street on Hudson Avenue, near the California Institute of Technology campus.

According to a statement released by the Pasadena Police Department, as officers were speaking with the driver of the truck, he suddenly sped away, narrowly missing hitting an officer. This reckless action led to a pursuit, with the driver now being wanted for assault with a deadly weapon on a police officer. The pursuit ended when Andrade crashed into the frontyard of a nearby home, colliding with a Tesla parked in the driveway. Ring doorbell camera footage captured the dramatic moment of impact, with the white truck plowing into the parked vehicle.

John Kelleher, a long-time resident of Pasadena, described hearing a loud crash that shook his home as Andrade’s truck careened through his front yard and struck the Tesla, pushing it into a neighbor’s fence. After crashing the vehicle, Andrade fled on foot and was eventually located in a nearby backyard. As a police dog attempted to apprehend him, Andrade brandished a handgun.

Despite orders to drop the weapon, Andrade failed to comply, and an officer-involved shooting ensued, resulting in his death. He was pronounced dead at a local hospital shortly after the incident. A handgun was recovered at the scene by authorities, further adding to the complexity and tragedy of the situation.

The events that transpired that night in Pasadena have left many residents shocked and saddened by the loss of life and the chaos that unfolded in their neighborhood. The Pasadena Police Department is conducting an investigation into the incident to determine the sequence of events leading up to the fatal shooting. In the meantime, the community is left grappling with the aftermath and seeking answers to the questions surrounding this tragic event.

As more details emerge and the investigation progresses, the hope is that a clearer picture will come to light, shedding light on the factors that contributed to this unfortunate turn of events. The impact of this incident will undoubtedly be felt by all those involved, from the officers who were forced to make split-second decisions to the family and friends of Ricardo Guade Andrade who are now left to grieve his loss.

In times like these, it is important for communities to come together, support one another, and seek understanding and healing in the face of tragedy. The road to healing will be long and challenging, but with unity and compassion, the community of Pasadena can begin to navigate through this difficult time and work towards a more peaceful and harmonious future.

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Further Support for Gravitational Wave Background in the Universe

The discovery of the gravitational wave background in 2016 marked a significant milestone in our understanding of the Universe. This groundbreaking discovery was further validated by the release of a second data set from the European Pulsar Timing Array, along with the addition of data from the Indian Pulsar Timing Array. These complementary studies have provided more evidence for the existence of the gravitational wave background, shedding light on the cosmic phenomena that shape our universe.

Gravitational waves are ripples in spacetime that are generated by violent processes such as merging black holes and colliding neutron stars. Predicted by Einstein in 1916 as part of his General Theory of Relativity, these waves have the ability to travel through space, largely unimpeded by any obstacles in their path. The first detection of gravitational waves in 2015 by the Laser Interferometer Gravitational-Wave Observatory (LIGO) confirmed their existence, originating from a gravitational merger between two black holes located 1.3 billion light years away.

The Laser Interferometer Gravitational-Wave Observatory is made up of two detectors, this one in Livingston, La., and one near Hanford, Wash. The detectors use giant arms in the shape of an “L” to measure tiny ripples in the fabric of the universe. Credit: Caltech/MIT/LIGO Lab

The recent confirmation of the gravitational wave background by the European and Indian Pulsar Timing Arrays indicates that we are detecting a combined signal from the mergers of supermassive black holes. This random distribution of gravity waves that permeates the Universe offers a new avenue for studying the cosmos, akin to the Cosmic Background Radiation. The collaborative efforts of various observatories and research institutions have enabled us to delve deeper into the mysteries of the Universe.

The full-sky image of the temperature fluctuations (shown as color differences) in the cosmic microwave background, made from nine years of WMAP observations. These are the seeds of galaxies, from a time when the universe was under 400,000 years old. Credit: NASA/WMAP

Utilizing pulsar timing arrays as galaxy-sized detectors, researchers have been able to monitor and analyze the pulse arrival times of galactic pulsars on Earth. By detecting subtle patterns in these signals, they can uncover the presence of the gravitational wave background. The latest study led by J. Antoniadis from the Institute of Astrophysics in Greece delves into the implications of the low-frequency signals observed in the recent data releases from various pulsar timing array systems.

The accumulation of data from multiple sources has provided undeniable evidence for the existence of the gravitational wave background. With ongoing Pulsar Timing Array projects, the signals of the low-frequency gravity waves will become more distinct, offering a wealth of opportunities to explore the Universe in this novel way. The focus now shifts towards interpreting these signals to unlock the secrets of the cosmos.

Source : The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

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