Category: 7. Science

  • Astronomy Guide: Sturgeon Moon 2025 to Light Up August Skies – Deccan Herald

    Astronomy Guide: Sturgeon Moon 2025 to Light Up August Skies – Deccan Herald

    1. Astronomy Guide: Sturgeon Moon 2025 to Light Up August Skies  Deccan Herald
    2. Attention stargazers! It’s time for one of the best meteor showers of the year — the Perseids  CBC
    3. What’s Up: August 2025 Skywatching Tips from NASA  NASA Science (.gov)
    4. Viewing the Perseids in 2025  American Meteor Society
    5. Sturgeon Moon 2025 rises this weekend. 6 reasons you should see the last full Moon of the summer  BBC Sky at Night Magazine

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  • Jim Lovell, Apollo 13 Commander, dies at age 97: How NASA’s legendary US astronaut led his crew through one of space’s greatest rescues |

    Jim Lovell, Apollo 13 Commander, dies at age 97: How NASA’s legendary US astronaut led his crew through one of space’s greatest rescues |

    James A. Lovell Jr., the famed astronaut and commander of NASA’s Apollo 13 mission, has died at 97. Lovell passed away on August 8, 2025, in Lake Forest, Illinois, his family confirmed in a statement to NASA. Though Lovell never walked on the Moon, his leadership during Apollo 13’s near-disastrous oxygen tank explosion turned the mission into one of space exploration’s greatest rescue stories. His calm, quick thinking under intense pressure saved the lives of his crew and inspired millions worldwide. Lovell’s heroism was immortalized in the 1995 film Apollo 13, where Tom Hanks portrayed him. Beyond his space legacy, Lovell remains a symbol of resilience and courage, admired by generations of astronauts and space enthusiasts alike.

    Jim Lovell’s early life and path to NASA

    Born March 25, 1928, in Cleveland, Ohio, James Arthur Lovell Jr. lost his father at a young age and was raised in Milwaukee by his mother. Fascinated by rocketry as a teenager, he even built a homemade gunpowder rocket—a passion that eventually shaped his career.After attending the University of Wisconsin–Madison for two years, Lovell entered the US Naval Academy, graduating in 1952. He went on to become a Navy test pilot before being selected in 1962 as part of NASA’s second group of astronauts, destined for the Gemini and Apollo programs.

    Jim Lovell record-breaking space career before Apollo 13

    Before Apollo 13, Lovell already held the record for most hours in space among astronauts of the Mercury, Gemini, and Apollo eras—logging over 715 hours.

    • Gemini 7 (1965) – Flew with Frank Borman on a 14-day mission, achieving the first space rendezvous.
    • Gemini 12 (1966) – Commanded the final Gemini mission with Buzz Aldrin, demonstrating critical spacewalking techniques.
    • Apollo 8 (1968) – Served as command module pilot on the first human mission to orbit the Moon, delivering the famous “plaster of Paris” description of its surface and witnessing the iconic Earthrise photograph.

    By the time Apollo 13 launched, Lovell was one of NASA’s most experienced astronauts.

    Jim Lovell, Apollo 13 mission journey

    Apollo 13 spacecraft damaged: The oxygen tank blast that changed NASA history

    Apollo 13 lifted off on April 11, 1970 with Lovell as commander, Fred W. Haise Jr. as lunar module pilot, and John L. “Jack” Swigert Jr. as command module pilot. The plan was for Lovell and Haise to land in the Fra Mauro highlands while Swigert orbited above.But 56 hours into the mission, roughly 200,000 miles from Earth, disaster struck. An oxygen tank in the service module exploded after a damaged wire ignited during a routine stir. The blast crippled the spacecraft—knocking out power, oxygen, and water supplies. It was then that the phrase—misquoted in popular culture as “Houston, we have a problem”—entered the American lexicon. In reality, Swigert first radioed, “Houston, we’ve had a problem,” with Lovell repeating it shortly afterward.

    Apollo 13 crisis management: How the lunar module saved the crew

    With the main command module crippled, the astronauts and NASA engineers devised an audacious survival plan—use the lunar module (LM) as a lifeboat. Designed for only two astronauts for two days, the LM now had to sustain three astronauts for four days.To conserve resources, they:

    • Powered down lights, heaters, and non-essential systems
    • Endured cabin temperatures of 38°F (3°C)
    • Survived on minimal rations, including hot dog packets for moisture
    • Built a makeshift carbon dioxide filter from duct tape, plastic bags, and a sock to keep the air breathable

    An immediate return to Earth was too risky, so Apollo 13 looped around the Moon for a slingshot trajectory home. Lovell manually guided crucial rocket burns using Earth’s position through the spacecraft window as a navigation point.

    Apollo 13’s safe return: From ocean rescue to Presidential honour

    On April 17, 1970, after one of the most tense survival stories in modern history, Apollo 13 splashed down safely in the Pacific Ocean, 610 miles southeast of American Samoa. Three orange-and-white parachutes signaled the end of the crisis. President Richard Nixon awarded Lovell, Haise, and Swigert the Presidential Medal of Freedom, calling the mission “a successful failure”—failed in its lunar landing but victorious in its safe return.Lovell co-authored the 1994 book Lost Moon: The Perilous Voyage of Apollo 13 with Jeffrey Kluger, which became the basis for Ron Howard’s hit film Apollo 13. In the movie, Tom Hanks played Lovell, immortalizing his calm leadership for a new generation.Lovell even made a cameo as the captain of the USS Iwo Jima, the recovery ship that retrieved the Apollo 13 crew.

    James Lovell’s life After NASA: Leadership, family, and lasting honours

    Lovell retired from NASA and the Navy in 1973, going on to lead the Bay-Houston Towing Company and hold senior roles in telecommunications. He also ran Lovell Communications, a Chicago-based consulting firm. His family operated a Lake Forest restaurant decorated with space memorabilia until it closed in 2015. Lovell is survived by his four children—James III (Jay), Jeffrey, Barbara, and Susan—11 grandchildren, and nine great-grandchildren. His wife of more than 60 years, Marilyn Lovell, died in 2023.In addition to the Presidential Medal of Freedom, Lovell was awarded the Congressional Space Medal of Honor by President Bill Clinton in 1995. In later years, Lovell often reflected that while missing the Moon was a disappointment, Apollo 13’s rescue was a greater triumph.“It was a triumph in a different direction—getting people back from a certain catastrophe,” he said.Also Read | NASA Hubble Space Telescope captures image of interstellar comet 3I/ATLAS speeding at 130,000 mph


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  • A novel method for assessing postmortem interval using radon radioisotopic decay – an internal radon ‘time of death clock’

    A novel method for assessing postmortem interval using radon radioisotopic decay – an internal radon ‘time of death clock’

    Conceptual framework

    We speculate that there is an opportunity to estimate PMI using the relative abundance of radioactive decay products generated from naturally occurring (^{222}textrm{Rn}) and that is absorbed by living systems. More specifically, the inhalation of radon gas and its decay products is functionally universal on Earth, as (^{222}textrm{Rn}) is generated by uranium isotope-bearing minerals within the lithosphere and migrates via free-phase gas and water to the surface, where it enters the atmosphere of including indoor and outdoor air environments occupied by people20,21. Human populations are exposed to some amount of radon and radon decay products daily, which is typically measured in an indirect manner by evaluating the amount of alpha particle emissions per second (Bq) per cubic metre of air ((Bq/m^3))22. (^{222}textrm{Rn}) levels in outside air are typically measured in the 1-60 (Bq/m^3) range23,24,25, although can be (>100) (Bq/m^3) in exceptional cases26. Indoor air or subterranean air radon amounts can be anything from 10-100,000 (Bq/m^3), depending on building and region20. (^{222}textrm{Rn}) has a relatively short half-life of 3.8 days before undergoing a series of radioactive decays to form a series of very short lived ((t_{1/2}) = microseconds to minutes) isotopes of Po, Pb and Bi before becoming long-lived (^{210}textrm{Pb}) ((t_{1/2}) = 22.3 years), then (^{210}textrm{Bi}) ((t_{1/2}) = 5 days), (^{210}textrm{Po}) ((t_{1/2}) = 138 days), and finally stable (^{206}textrm{Pb}) (Figure 1).

    Although exposure to some amount of gaseous (^{222}textrm{Rn}) and solid radon decay products is functionally universal, the specific amount of these radioisotopes inhaled by a person occurs at variable amounts across a lifetime depending on where they live, in what buildings they occupy, and behavioural factors such as occupation, tobacco use, diet and more27,28,29,30,31. It is important to understand that human exposure to radon and its decay products is a function of how much gaseous (^{222}textrm{Rn}) is constantly entering a given environment from geogenic sources, and also those radon-decay products that have equilibrated within the same environment via (^{222}textrm{Rn}) decay and attachment to particulates such as smoke or dust20. Both gaseous radon and the ‘attached fraction’ of radon decay products are inhaled and will be absorbed into living tissue via the lungs32,33,34. To a lesser extent, radon and its decay products can be ingested via drinking groundwater, eating certain foods such as (^{210}textrm{Pb})-rich lichen-eating wild game (e.g. caribou, elk, deer, moose), or tobacco smoking34,35,36. As all these routes of exposure demand that a person is alive, the deposition of (^{222}textrm{Rn}) and radon decay products within tissue is innately associated with life, whilst the cessation of breathing, drinking, and/or eating that occurs at death marks the end of incoming (^{222}textrm{Rn}) and radon decay products.

    Careful measurement of the relative abundance of these decay products is now possible using recent advances in technology and so, for the first time, it is theoretically possible to use a radioisotopic decay of (^{222}textrm{Rn}) to evaluate PMI. Indeed, previous work by Ziad and colleagues37 explored the use of radon decay product ratio measurements to estimate time of death. Assumptions made during that investigation included constant radon exposure during life and an initial equilibrium value of (^{210}textrm{Pb}):(^{210}textrm{Po}) that complicates time of death estimation37; as these assumptions were undefined, they added uncertainties. We note that while the theoretical idea to measure (^{222}textrm{Rn}) decay products to estimate PMI is straightforward, its practical application is not. The accumulation of radon decay products in tissue is in the order of femtogram per gram (fg/g). Consequently, hypersensitive instruments are needed to measure isotope abundance (i.e. number of atoms) of radon decay products in biological tissues. If a low abundance measuring procedure is in place, as has been achieved for uranium or plutonium isotopes38, the next problem is to identify tissues that are helpful to measure within the context of a corpse, based how radon decay products are stored in the body. Current evidence suggests that, in addition to the lungs, keratinizing tissue (nails), adipose tissue (fat), and bone are all tissues where radon decay products have been empirically found to accumulate33,34. To develop and evaluate a theoretical model, we divided our work into two consecutive phases: the forward model and the actual Radon Time of Death Clock calculation. Our rationale was to use the radioactive decay equations under the assumption of a steady source of radon to generate data that could then be used to test the accuracy of the Radon Time of Death Clock. A critical component of the Radon Time of Death Clock developed here is the use of (1) relative numbers of isotopes and (2) two pairs of isotope abundance ratios. These input data enable a determination of the elapsed time since death to very high accuracy and is a key feature of this approach.

    The forward model

    For the forward model, we conceptualized a person who inhaled air containing an average of 100 (Bq/m^3) radon from birth to the time at which they died (time of death = (t_d)). The radon exposure assumption reflects the reality of radon in many nations including, for example, Canada where recent outcomes of national surveying found that the geometric mean, weighted level of radon in a residential building is 84.7 (Bq/m^3), with 42(%) of people experiencing levels of radon 100 (Bq/m^3) or more. For the forward model, we also assumed inhalation of radon and all radon decay products ceased entirely at the time of death, and that the numbers of (^{210}textrm{Pb}), (^{210}textrm{Bi}), and (^{210}textrm{Po}) atoms each began to decrease according to radioactive decay laws and their respective radioisotopic decay probabilities. At specific times after the discovery of the theoretical corpse by investigating authorities, we assumed the measurements of radon decay products in one or more tissues from the body could be performed (time of measurement = (t_m)), including the numbers of remaining atoms and isotope number ratios.

    We suggest that two ratios that involve three radon decay isotopes ((^{210}textrm{Pb}), (^{210}textrm{Bi}), and (^{210}textrm{Po})) are of particular interest, as these isotopes have relatively longer half-lives; these ratios are: (r_1 = frac{^{210}textrm{Pb}}{^{210}textrm{Po}}) and (r_2 = frac{^{210}textrm{Pb}}{^{210}textrm{Bi}}). Starting with zero atoms for all the species of interest, and having a set of decay rates, we can obtain the ratios of the number of atoms at any time before or after death. The decay equations guarantee existing a unique set of ratios for any specific set ({t_d, t_m}),

    $$begin{aligned} begin{aligned}&hbox {d}{N_{0}}{t} = A – lambda _0 N_{0},\&hbox {d}{N_{1}}{t} = lambda _0 N_{0} – lambda _1 N_{1},\&hbox {d}{N_{2}}{t} = lambda _1 N_{1} – lambda _2 N_{2},\&hbox {d}{N_{3}}{t} = lambda _2 N_{2} – lambda _3 N_{3}, end{aligned} end{aligned}$$

    (1)

    In this scenario, the value A (Bq) represents the constant activity level of radon in air, and ((lambda _0, N_{0})), ((lambda _1, N_{1})), ((lambda _2, N_{2})), ((lambda _3, N_{3})) denote decay constants and number of atoms for (^{222}textrm{Rn}), (^{210}textrm{Pb}), (^{210}textrm{Bi}) and (^{210}textrm{Po}), respectively. However, after death, the first equation follows:

    $$begin{aligned} hbox {d}{N_{0}}{t} = – lambda _0 N_{0}, end{aligned}$$

    (2)

    In this scenario, the supply of radon to the body ceases, the (^{222}textrm{Rn}) atoms undergo decay and, since the person is no longer inhaling air, there is no source to replenish the (^{222}textrm{Rn}) atoms. Below are the solutions to the above equations before death:

    $$begin{aligned} N_{1}(t)= frac{A lambda _0 (1- e^{-lambda _1 t})}{lambda _1}, end{aligned}$$

    (3)

    $$begin{aligned} N_{2}(t)= frac{A lambda _0 (lambda _1 (1-e^{-lambda _2 t})+lambda _2 (e^{-lambda _1 t}-1))}{(lambda _1-lambda _2) lambda _2}, end{aligned}$$

    (4)

    $$begin{aligned} begin{aligned} N3(t)= frac{A lambda _0 e^{-(lambda _1+lambda _2+lambda _3) t}}{(lambda _1-lambda _2) (lambda _1-lambda _3) (lambda _2-lambda _3) lambda _3}times&[(lambda _1^2 e^{lambda _1 t} (lambda _2 e^{lambda _2 t} (e^{lambda _3 t}-1)-lambda _3 e^{lambda _3 t} (e^{lambda _2 t}-1)) \&+lambda _1 e^{lambda _1 t} (lambda _3^2 e^{lambda _3 t} (e^{lambda _2 t}-1)-lambda _2^2 e^{lambda _2 t} (e^{lambda _3 t}-1))\&+lambda _2 (lambda _2-lambda _3) lambda _3 e^{(lambda _2+lambda _3) t} (e^{lambda _1 t}-1))]. end{aligned} end{aligned}$$

    (5)

    A Monte Carlo simulation was done where the age of the individual and the time that elapsed between death ((t_d)) and the measurement ((t_m)) were varied. Specifically, (t_{d}) varied between 20 and 40 years and (t_m) varied up to 20 days. The simulation was run 3,500 times to create multiple sets of (frac{^{210}textrm{Pb}}{^{210}textrm{Bi}}) and (frac{^{210}textrm{Pb}}{^{210}textrm{Po}}) isotope number ratios, with each pair having a known (t_{d}) and (t_{m}).

    Fig. 1

    The (^{222}textrm{Rn}) main decay chain and daughter products. The half-life of each isotope is indicated. Only the dominant decay pathways are shown and low-probability branches (e.g., (^{218}textrm{Po}) to (^{218}textrm{At})) are omitted for clarity.

    The radon time of death clock

    We next used the data generated from Monte Carlo simulations as input quantities to the Radon Time of Death Clock, to test its theoretical accuracy, meaning how well outcomes predicted a known time of death. The calculation of the elapsed time for measuring the numbers of (^{210}textrm{Pb}), (^{210}textrm{Bi}), and (^{210}textrm{Po}) atoms ((t_{m})) was based only on the relative isotope number ratios. Thus, the input quantities to the Radon Time of Death Clock were the (r_1) and (r_2) ratios. Here, we assumed the individual was exposed to a constant level of radon over their lifetime. The model was implemented in Python 3.0 and employs the “brute force” method that involved calculating the function’s value at each point on a multidimensional grid to determine the function’s global minimum, and the Nelder-Mead minimization algorithm to calculate the elapsed times between death and measurement of isotopic composition.

    The model solved the radioactive decay equations simultaneously for the two pairs of number ratios such that, although the radioactive decay probabilities for each radionuclide are different, the elapsed time for radioactive decays must be the same. Very importantly – as it would be impractical in the field – knowledge of the absolute radon exposure of the person at the time of death was not needed, as this quantity was cancelled out in the calculation since equations employed the relative number of isotopes (i.e. (^{210}textrm{Pb}) to (^{210}textrm{Bi}) and (^{210}textrm{Pb}) to (^{210}textrm{Po})). The use of two sets of the relative numbers of isotopes enabled the calculation of a unique answer. In the case of using a single isotope number ratio in the calculation (i.e. only (^{210}textrm{Pb}) to (^{210}textrm{Bi})), the result from the model was not unique. However, if both relative isotope number ratios were input to the model, then the result was constrained to a much narrower range of possible values for the time elapsed between death and measurement, where a solution to the equations is found.

    Constant lifetime radon exposure

    In the hypothetical scenario of constant radon exposure during a lifetime, we define a two-dimensional vector field, (vec {r} = vec {S}(t_d, t_m)), where (vec {r} = (r_1, r_2)). Vector field (vec {S}) can be evaluated based on decay equations for any valid set ({t_d, t_m}), either analytically or numerically. We consider evaluating vector field (vec {S}) at any given time set to be ‘solving the direct problem’ – i.e., solving the direct problem simulates a reality in which a person lived for a specific time with a constant radon exposure, died at (t_d), and the (r_1) and (r_2) ratios are measured at (t_d + t_m). The components of (vec {S}(t_d, t_m)) give us the ratio values in the ideal case of no uncertainty in the measurement results.

    Assuming that there is a unique set of times, ({t_{d,T}, t_{m,T}}), which leads to a specific set of measured ratios, ({r_{1,T}, r_{2,T}}) (i.e. (vec {r}_T = (r_{1,T}, r_{2,T}) = vec {S}(t_{d, T}, t_{m, T}))) that we define ’solving the inverse problem’ as follows. The subscript T denotes the true value, which is presumed to be measured. Due to the absence of uncertainty, this true value should correspond to the value obtained from the forward model. When defining the scalar field,

    $$begin{aligned} E_{vec {r}_T}(t_d, t_m) = left| vec {S}(t_d, t_m) – vec {r}_Tright| , end{aligned}$$

    (6)

    we suggest that there should be one single global minimum for (E_{vec {r}_T}) which happens at ((t_{d, T}, t_{m, T})). Hence, for a given set of valid ratios, (vec {r}_T), one can find the set of times, ({t_{d, T}, t_{m, T}}), that leads to the measured ratios, by minimizing the scalar field (E_{vec {r}_T}).

    To test the accuracy of the model, we next calculated the elapsed time since death for the isotope pairs produced by the Monte Carlo simulations. The results are shown in Figure 2a, where the difference between actual and calculated elapsed measurement times (optimization error) are plotted as a function of the time that has elapsed since death. Outcomes demonstrate that the Radon Time of Death Clock could provide reliable results within just a two-week window after actual the death of the individual, and were remarkably precise with the average absolute error of 114 milliseconds. The consistency of the results was supported by a standard deviation of approximately 141 milliseconds. The error distribution arising from a scenario involving constant radon exposure and a single time measurement of two isotope pairs is shown in Figure 2b.

    Fig. 2
    figure 2

    (a) Difference between the true and calculated elapsed time since death using the two pairs of isotope number ratios. Note that no uncertainty was assumed for the input quantities to the model. The RTDC could calculate the accurate time of death to within seconds. (b) Distribution of errors in post-mortem interval estimation under constant radon exposure conditions, showing Gaussian distribution pattern of discrepancy between predicted and actual time since death.

    Accounting for variation in radon exposure across a lifetime

    In reality, people are exposed to (^{222}textrm{Rn}) and solid radon decay products at a variable rate and at different levels across their lifespan20,21,28,39. Empirical evidence for ever changing radon exposure across a lifetime exists and has been demonstrated, with shifts in exposure caused by life events such as entering the workforce, changing profession, starting or stopping tobacco smoking, moving house, entering retirement, obtaining a radon reduction, and/or more systemic events such as implementation of pandemic emergency lockdown responses telecommuting, or nation wide building code changes27,28,29,30,31. So, to make the model more realistic, we next modeled a scenario where we assumed that the rate of radon exposure undergoes multiple changes during individual’s lifespan (albeit, for simplicity, each period of exposure was constant between jumps).

    Similar to the case of constant exposure, we define the vector field (vec {r} = vec {S}_{f(t)}(t_d, t_m)), where f(t) is a piece-wise constant function of time that gives the overall rate of radon exposure activity over time. Note that the rate of radon exposure activity is defined only within the time between conception and death and that, after death, all relevant radionuclides will decay with no further input from parental (^{222}textrm{Rn}) and/or solid radon decay products. Therefore, all the discontinuities of f(t) should satisfy (0, and (f(t)=0) for (t>t_d). Furthermore, for a constant function f(t) within (0, we have, (vec {S}_{f(t)} = vec {S}). Mathematically, we define,

    $$begin{aligned} f(t) = {left{ begin{array}{ll} a_1 quad quad quad & ,0< t< t_1\ a_2 & ,t_1< t< t_2\ vdots \ a_N & ,t_{N-1}< t< t_N\ a_{N+1} & ,t_N< t< t_d\ 0 & ,t_d < t end{array}right. }, end{aligned}$$

    (7)

    Here, N is the number of jumps in the rate of radon exposure activity the person experiences, while (t_n in T_{jumps}) is the time of (n^{th}) jumps, and (a_j in jumps) is the constant value describing the rate of radon exposure activity between two successive jumps.

    In an ideal scenario, solving the inverse problem would determine the set of parameters ({t_d, N, jumps, T_{jumps}, t_m}), in which N is the number of jumps, jumps, is the set of activity values between the jumps, and (T_{jumps}) is the set of times of jumps before (t_d), such that these lead to a set of ratios that match with the measured values in reality (or the outcome of (vec {S}_{f(t)}(t_d, t_m))). However, from a practical perspective, solving such a problem would far too computationally expensive to be helpful (i.e., impractical using regular computers, as the number of unknown parameters is large). It can be claimed that if there is any piece-wise constant function (tilde{f}(t) ne f(t)) and (tilde{t}_dne t_d) such that,

    $$begin{aligned} vec {S}_{tilde{f}(t)}(tilde{t}_d, 0) simeq vec {S}_{f(t)}(t_d, 0), end{aligned}$$

    (8)

    Then will have the equation below for any (t_m):

    $$begin{aligned} vec {S}_{tilde{f}(t)}(tilde{t}_d, t_m) simeq vec {S}_{f(t)}(t_d, t_m), end{aligned}$$

    (9)

    The implication of this is that the post-mortem evolution of these radioisotopic ratios is predicted to follow a similar pattern regardless of the lifespan or lifetime radon exposure of the person, meaning this readout of PMI is agnostic to inter-individual differences, and so is likely helpful to forensic investigators who need to ascertain PMI. To move forward with evaluation our model, we proceeded under the assumption that it is feasible to replicate the post-mortem characteristics of (r_1) and (r_2) from a scenario with the death occurring at time (t_d) and multiple fluctuations in the rate of radon exposure activity over the lifespan. We used a less complex scenario where death happens at a different time (t_d^prime) ((t_d ne t_d^prime)) and involves a single change in rate of radon exposure activity. Although this approach is an approximation and will not exactly mirror the reality of lifetime radon exposure, it is a reasonable estimation for a wide range of cases. To formulate the aforementioned approximation, we initially define a step-function g(t) as follows,

    $$begin{aligned} g(t) = {left{ begin{array}{ll} a_1 quad quad quad & , 0< t< t_1\ a_2 & , t_1< t< t_d\ 0 & , t_d < t end{array}right. }. end{aligned}$$

    (10)

    Since we deal with the ratios, the absolute values of (a_1) and (a_2) do not affect the results directly, rather, the ratio (a = a_2/a_1) is what is important for us. So, we redefine the function g(t) to reduce the number of parameters,

    $$begin{aligned} g(t) = {left{ begin{array}{ll} 1 quad quad quad & , 0< t< t_1\ a & , t_1< t< t_d\ 0 & , t_d < t end{array}right. }. end{aligned}$$

    (11)

    Now, with having (vec {r}_T = vec {S}_{f(t)}(t_{d, T}, t_{m, T})), we define the scalar field,

    $$begin{aligned} E_{vec {r}_T}(t_d, t_m, t_1, a) = left| vec {S}_{g(t)}(t_d, t_m) – vec {r}_Tright| . end{aligned}$$

    (12)

    Similar to the case of constant activity, by minimizing the scalar field (E_{vec {r}_T}), we can obtain the set of parameters that result in the ratios of interest, and those parameters include (t_m).

    Measurement of radioisotope ratios at multiple times postmortem

    The theoretical approach we have described so far yields generally satisfactory outcomes. However, in certain instances, we observed that it can lead to very large uncertainty on (t_m) values. The discrepancy arises because the parameters ({t_d, t_m, t_1, a}) that result in (vec {r}_T) are not unique, and an example where the method fails is depicted in Figure 3.

    Fig. 3
    figure 3

    This figure demonstrates how minimization is used to estimate the time of death based on forward model data. A single postmortem measurement, which did not match accurately the true time of death, was also analyzed using double measurement approaches. Under lifetime-varying radon exposure, the minimization curve deviates from the forward model (true ratio curve) when using a single postmortem measurement. In contrast, the dashed line representing the double measurement approach closely matches the forward model. (a) shows the minimization result for isotope ratio (r_{1}(frac{^{210}textrm{Pb}}{^{210}textrm{Po}})) and (b) the minimization result for isotope ratio (r_{2}(frac{^{210}textrm{Pb}}{^{210}textrm{Bi}})).

    In all cases, the resulting ratios match those obtained from the forward model simulation. However, there is a notable discrepancy in the estimation of (t_m). To address this issue, one approach we suggest is to incorporate radioisotope ratios with their rates of change (time derivative) into the analysis. As an approximation of the time derivative, a second measurement of ratios can be introduced into the scenario. The first measurement takes place at (t_{1,T} = t_{d,T} + t_{m,T}), and the second measurement at the time (t_{2,T} = t_{d,T} + t_{m,T} + t_text {step}). The outcomes are denoted as (vec {r}_{1,T} = (r_{1,1,T}, r_{2,1,T})) for the first measurement and (vec {r}_{2,T} = (r_{1,2,T}, r_{2,2,T})) for the second one.

    $$begin{aligned}&vec {r}_{1,T} = vec {S}_{f(t)}(t_{d, T}, t_{m, T}), end{aligned}$$

    (13)

    $$begin{aligned}&vec {r}_{2,T} = vec {S}_{f(t)}(t_{d, T}, t_{m, T} + t_text {step}). end{aligned}$$

    (14)

    Then we define the scalar field that should be minimized as,

    $$begin{aligned} begin{aligned} E_{vec {r}_{1,T},vec {r}_{2,T}}(t_d, t_m, t_1, a) =&left| vec {S}_{g(t)}(t_d, t_m) – vec {r}_{1,T}right| + left| vec {S}_{g(t)}(t_d, t_m+t_text {step}) – vec {r}_{2,T}right| . end{aligned} end{aligned}$$

    (15)

    The error distribution for a model with varying radon exposure and two measurements of two isotope pairs that are separated in time is in Figure 4. Since no measurement of isotopic composition is free from uncertainty, a preliminary study was carried out to explore the sensitivity of the Radon Time of Death Clock to measurement errors. An initial run introduced random error to the the (r_1) and (r_2) isotope number ratios and the model calculations were repeated using a relative standard deviation of 0.01 percent in the ratios. Under these conditions, the uncertainty in the elapsed time calculation increased to approximately 1 day. To explore the theoretical limit of the model’s temporal resolution, calculations were repeated assuming a relative uncertainty of 0.01(%) in the isotope ratios. While this level of precision is not currently achievable using standard detection techniques, it serves as an upper-bound scenario to evaluate model behavior under idealized conditions, such as might become accessible through future advances in measurement technology.

    Fig. 4
    figure 4

    (a) Difference between the true and calculated elapsed time since death using two pairs of isotope ratios. The study employed a double measurement approach, where two pairs of isotopes were measured twice at separate time intervals. Note that no uncertainty was assumed for the input quantities to the model. The RTDC could calculate the accurate time of death to within 10 minutes. (b) Distribution of optimization errors in post-mortem interval estimation under varying radon exposure conditions, showing Gaussian distribution pattern of discrepancy between predicted and actual time since death.

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  • Time-Lapse Of SpaceX CRS-32 Dragon Cargo Spacecraft Approaching ISS – MSN

    1. Time-Lapse Of SpaceX CRS-32 Dragon Cargo Spacecraft Approaching ISS  MSN
    2. “We Brought the Future Back to Earth” Declares SpaceX After Dragon Lands With 6,700 Pounds of Advanced Robots From Wild Mission  Rude Baguette
    3. Watch NASA’s SpaceX Crew-10 Dock With Space Station In This Time-Lapse  MSN
    4. Time-Lapse: SpaceX Dragon And The Milky Way Seen From ISS  MSN

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  • Strange faces, canals and Earth invaders: five fantastical visions of Mars that exist only in our imagination

    Strange faces, canals and Earth invaders: five fantastical visions of Mars that exist only in our imagination

    Mars continues to fascinate us. Early stargazers saw it only as a small, red pinprick of light, then the advent of telescopic astronomy gave us views of its surface features and seasonal changes.

    The dawn of Space Age meant we could send rovers and orbiters to the surface of Mars for the first time, unravelling the mysteries of its ancient history and finding proof that liquid water once flowed on its surface.

    Credit: ESA/DLR/FU Berlin/G. Michael

    We may even be getting closer to deciphering whether Mars once had life on its surface.

    Unsurprisingly, myths about Mars abound, both old and new.

    Here are five strange – and completely untrue – visions of the Red Planet.

    Lowell’s canals

    Gullies and channels on Mars. Credit: NASA
    Gullies and channels on Mars. Are these the ‘canals’ that early astronomers thought they saw? Credit: NASA

    Percival Lowell and others interpreted strange linear markings on Mars as canals engineered by sentient Martians.

    This was likely the result of Italian astronomer Giovanni Schiaparelli’s observations of Mars, and his report of seeing ‘canali’ on the planet, which means ‘channels’, but was mis-translated into English as ‘canals’.

    Future observations disproved the Mars ‘canals’ as an optical illusion, but author CS Lewis said the canals became “part of the popular tradition”.

    Mariner 4’s fly-by in 1965 conclusively disproved their existence.

    War of the Worlds

    Illustration of Martians attacking from a 1906 edition of The War of the Worlds by H.G. Wells. Credit: Bettmann / Getty Images
    Illustration of Martians attacking from a 1906 edition of The War of the Worlds by H.G. Wells. Credit: Bettmann / Getty Images

    HG Wells’ 1898 War of the Worlds presented Martians with an inhuman appearance.

    Inspired by 19th-century British colonialism and its devastating effect upon Aboriginal Tasmanians, Wells inverted the idea of aliens from beneficent beings of higher intelligence into fearsome, warlike creatures.

    Orson Welles’ radio broadcast

    Orson Welles rehearsing his radio adaptation of H.G. Wells' classic, 'The War of the Worlds', 10th October 1938. Credit: Bettmann / Getty Images
    Orson Welles rehearsing his radio adaptation of H.G. Wells’ classic, ‘The War of the Worlds’, 10th October 1938. Credit: Bettmann / Getty Images

    In 1938, Orson Welles narrated an adaptation of War of the Worlds for CBS.

    Presented as a simulated radio broadcast, with newsflashes and eyewitness accounts, its description of a Martian invasion won 23-year-old Welles fame as an innovative storyteller.

    It also became notorious due to the panic it induced among listeners.

    The Face on Mars

    Left: the original 'face on Mars' image captured by NASA's Viking 1 Orbiter spacecraft on 25 July 1976. Right: A more recent image of the same feature by the Mars Global Surveyor's Mars Orbital Camera on 8 April 2001 shows it doesn't really look like a face at all. Credit: NASA/JPL
    Left: the original ‘face on Mars’ image captured by NASA’s Viking 1 Orbiter spacecraft on 25 July 1976. Right: A more recent image of the same feature by the Mars Global Surveyor’s Mars Orbital Camera on 8 April 2001 shows it doesn’t really look like a face at all. Credit: NASA/JPL

    First imaged by the Viking 1 orbiter in 1976, the Face on Mars is in the Cydonia region of Mars’s northern hemisphere.

    At around 2km (1.2 miles) long, this mesa resembles a human face when viewed under certain conditions.

    But the ‘face’ is a mere trick of light and shadow, much like clair-obscur effects on the Moon, appearing as a natural rock formation when seen from other angles.

    Mars gremlins

    The Beagle 2 spacecraft landed on the surface of Mars but its solar panels failed to deploy, preventing communication. Credit: HIRISE/NASA/Leicester
    The Beagle 2 spacecraft landed on the surface of Mars but its solar panels failed to deploy, preventing communication. Credit: HIRISE/NASA/Leicester

    In 60 years of robotic exploration of Mars, half of all missions have ended badly due to launch failures, communication losses, explosions, software bugs or crash landings.

    These were colloquially attributed to ‘Mars gremlins’, honouring the mischievous folklore figures who delight in causing malfunctions in machinery.

    What are your favourite Mars myths? Let us know by emailing contactus@skyatnightmagazine.com

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  • The Sky Today on Saturday, August 9: A Full Sturgeon Moon rises – Astronomy Magazine

    1. The Sky Today on Saturday, August 9: A Full Sturgeon Moon rises  Astronomy Magazine
    2. What’s Up: August 2025 Skywatching Tips from NASA  NASA Science (.gov)
    3. Viewing the Perseids in 2025  American Meteor Society
    4. August full moon 2025 rises this weekend: Here’s how to see the stunning ‘Sturgeon Moon’  Space
    5. Preliminary hearing continues for Deandre Booker, man accused of killing Ashley Elkins  yahoo.com

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  • New signs found of giant gas planet in ‘Earth’s neighbourhood’

    New signs found of giant gas planet in ‘Earth’s neighbourhood’

    LONDON  –  Scientists have found strong evidence of a giant gas planet in the nearest star system to our own. At four-and-a-half light years away, the lifeless planet would be a close neighbour to Earth in astronomical terms and could have moons that sustain life. The signs were found in the star system Alpha Centauri by the powerful James Webb Space Telescope.

    The potential planet was detected last year, but it had disappeared in follow-up observations. Astronomers must now look again to prove it definitely exists.

    Scientists are particularly excited about this discovery because of the similarities between the exoplanet’s star and our Sun. “Four years is a long way but in galaxy terms, it’s very close – it’s in our neighbourhood,” said Dr Carly Howett, associate professor of space instrumentation at the University of Oxford. “It is around a star that is Sun-like and about the same temperature and brightness. That’s really important if we want to think about habitable worlds,” she added.

    The planet would be similar to our solar system’s gas giants, Saturn and Jupiter, and would be enveloped in a thick gas cloud. That means it could not support life itself, but it could have moons that are habitable.

    Jupiter and some other planets in our solar system have icy moons, which researchers believe could support life. Scientists are currently investigating that possibility on missions called Europa Clipper and Juice.  But those planets are far away from our life-giving Sun. The potential “new” planet is comparatively close to its star. The signs were found in direct imaging by the James Webb Space Telescope, which is the closest thing scientists have to taking photographs of distant objects. “These are incredibly challenging observations to make, even with the world’s most powerful space telescope, because these stars are so bright, close, and move across the sky quickly,” said Charles Beichman from Nasa’s Jet Propulsion Laboratory and co-first author of the new discoveries. Those stars create huge amounts of bright light that can block out nearby objects. That could be why the planet was detected once, in August 2024, but then seemingly disappeared when scientists looked for it again. “Probably the planet was either behind the star or too close to be able to see it. You need an element of luck,” said Dr Howett. Astronomers will now look for more signs of the planet. They hope to use a new Nasa telescope – the Grace Roman Space Telescope – which is due to start operating in 2027.

    Future observations by the James Webb Space Telescope should also be able to tell us what the planet is made up of, using something called spectral imaging.

    That will build up a more detailed picture of what it looks like, and how habitable any orbiting Moons could be.


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  • When Mars Looks Like Home: Perseverance’s “Falbreen” Panorama – DIYPhotography

    1. When Mars Looks Like Home: Perseverance’s “Falbreen” Panorama  DIYPhotography
    2. NASA’s Perseverance Rover Captures Mars Vista As Clear As Day  NASA Jet Propulsion Laboratory (JPL) (.gov)
    3. Earth or Mars? See the ‘deceptively’ clear blue sky spotted on the Red Planet  FOX Weather
    4. NASA’s six-wheeled scientist captures its best Mars panorama yet  Digital Trends
    5. NASA’s Perseverance Snaps One Of Sharpest 360° Panoramas On Mars Ever Taken  IFLScience

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  • Moon phase today explained: What the moon will look like on August 9, 2025

    Moon phase today explained: What the moon will look like on August 9, 2025

    The full moon is finally here, and if you’re lucky enough to be graced with a cloudless night, there’s a lot to see as we enter the next phase of the lunar cycle.

    This is a series of eight unique phases of the moon’s visibility. The whole cycle takes about 29.5 days, according to NASA, and these different phases happen as the Sun lights up different parts of the moon whilst it orbits Earth. 

    So, what’s happening with the moon tonight, Aug. 9?

    What is today’s moon phase?

    As of Saturday, Aug. 9, the moon phase is Full Moon, and it is 100% lit (NASA’s Daily Moon Observation confirms this).

    This month’s full moon is known as the Sturgeon Moon, an ode to fishing tribes and the plentiful sturgeon fish that was caught in the month of August.

    There’s so much to be seen on the moon’s surface tonight, but pay particular attention to the Mare Vaporum, the Mare Fecunditatis, and the Mare Tranquillitatis, all of which can be seen with the naked eye.

    When is the next full moon?

    The next full moon will be on September 7.

    Mashable Light Speed

    What are moon phases?

    According to NASA, moon phases are caused by the 29.5-day cycle of the moon’s orbit, which changes the angles between the Sun, Moon, and Earth. Moon phases are how the moon looks from Earth as it goes around us. We always see the same side of the moon, but how much of it is lit up by the Sun changes depending on where it is in its orbit. This is how we get full moons, half moons, and moons that appear completely invisible. There are eight main moon phases, and they follow a repeating cycle:

    New Moon – The moon is between Earth and the sun, so the side we see is dark (in other words, it’s invisible to the eye).

    Waxing Crescent – A small sliver of light appears on the right side (Northern Hemisphere).

    First Quarter – Half of the moon is lit on the right side. It looks like a half-moon.

    Waxing Gibbous – More than half is lit up, but it’s not quite full yet.

    Full Moon – The whole face of the moon is illuminated and fully visible.

    Waning Gibbous – The moon starts losing light on the right side.

    Last Quarter (or Third Quarter) – Another half-moon, but now the left side is lit.

    Waning Crescent – A thin sliver of light remains on the left side before going dark again.

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  • Watch SpaceX’s Crew-10 astronauts return to Earth today after nearly 5 months in space

    Watch SpaceX’s Crew-10 astronauts return to Earth today after nearly 5 months in space

    NASA’s SpaceX Crew-10 Re-Entry and Splashdown – YouTube


    Watch On

    SpaceX’s Crew-10 astronauts will return to Earth today (Aug. 9) after living on the International Space Station for nearly five months, and you can watch the action live.

    The mission’s Crew Dragon capsule, named Endurance, is scheduled to splash down in the Pacific Ocean off the California coast today at 11:33 a.m. EDT (1533 GMT; 8:33 a.m. local California time).

    You can watch the homecoming live here at Space.com, courtesy of NASA, or directly via the space agency. Coverage will begin at 10:15 a.m. EDT (1415 GMT).

    a white space capsule descends toward the ocean under four white and red parachutes

    SpaceX’s Crew-9 astronaut mission returns to Earth off the coast of Tallahassee, Florida on March 18, 2025. (Image credit: NASA TV)

    As its name suggests, Crew-10 is the 10th operational astronaut mission that SpaceX has flown to and from the International Space Station (ISS) for NASA, via the agency’s Commercial Crew Program (CCP).

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