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Honeycutt starred at UCLA and played for the Sacramento Kings

Honeycutt, a 6-foot-8 forward from Sylmar, just north of Los Angeles, played two seasons at UCLA from 2009-2011 and earned first-team All-Pac 12 honors in his sophomore season. He then declared for the NBA draft and was selected by Sacramento in the second round (35th overall pick) in 2011.

He played minimally for the Kings and was eventually traded to Houston in 2013. He never played for the Rockets, and in August, 2013, he moved his playing career overseas, starting with Ironi Nes Ziona in Israel. For the past few years, he had bounced back and forth between Khimki and Anadolu Efes in Turkey.

Honeycutt’s coach at Khimki, Giorgios Bartzokas, was too overwhelmed to comment, saying“I am sorry I cannot talk right now, I am really sad.”

“I am sorry i cannot talk right now, i am really sad” GBartzokas. Tyler Honeycutt, massa jove per morir.

— Víctor Lavagnini (@victorlavagnini)

Many NBA players — both current and past — expressed their thoughts on Twitter.

Still can’t believe this… Rest In Peace to my brother Tyler Honeycutt

— That Boy Jrue (@Jrue_Holiday11)

hurt by the news, glad no one else was injured, but ultimately sad to say, rest in peace to my basketball brother tyler honeycutt…

— Solomon Hill (@solohill)

R.I.P. Tyler Honeycutt

— Terrence Ross (@TFlight31)

RIP Tyler Honeycutt🙏🏾

Prayers up for his family and friends. Rest easy bro!

— DeMarcus Cousins (@boogiecousins)

RIP tyler honeycutt

— Spencer Dinwiddie (@SDinwiddie_25)

Wow. RIP to Tyler HoneyCutt. Former Teammate Good Friend. Thoughts and Prayers to His Family!

— Jason Thompson (@jtthekid)

My prayers go out to Tyler Honeycutt never know what ppl are going thru.

— Joe Crawford (@JoeCrawford5)

Rest Easy Tyler Honeycutt.. prayers up for him and family.. devastating.. just saw him yesterday..

— Quincy Pondexter (@QuincyPondexter)

Rest Easy Young King …Tyler Honeycutt … Extremely Sad News..

— DaJuan Summers (@DSummersTime)

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Age 7 to 18

Published May 2008,February 2011.

As the sun moves across the sky, shadows change in direction and length, so a simple sundial can measure the length of a day. It was quickly noticed that the length of the day varies at different times of the year. The reasons for this difference were not discovered until after astronomers accepted the fact that the earth travels round the sun in an elliptic orbit, and that the earth's axis is tilted at about 26 degrees. This variation from a circular orbit leads to the Equation of Time (see 'Note 2' below) which allows us to work out the difference between 'clock' time and 'sundial time'.
Another discovery was that sundials had to be specially made for different latitudes because the Sun's altitude in the sky decreases at higher latitudes, producing longer shadows than at lower latitudes. Today, artists and astronomers find many ways of creating modern sundials.
An Egyptian sundial from about 1,500 BCE is the earliest evidence of the division of the day into equal parts, but the sundial was no use at night. The passage of time was extremely important for astronomers and priests who were responsible for determining the exact hour for the daily rituals and for the important religious festivals, so a water clock was invented.
When you think about the problem - we can find due South easily from the sun at midday. Looking at the night sky, we eventually deduce that there is a fixed point in the heavens around which all the stars rotate once every day (24 hours). This is where we find the 'Pole Star' (from the Great Bear or Ursa Major, measure the distance of about four lengths of the two stars at the end, 'the pointers' to find Polaris). This is the Celestial Pole - which was different for the Egyptians from today because of the phenomenon of Precession.

Up to about 1,900 BCE the Celestial Pole was Thuban a star in the 'tail' of the constellation Draco. By 1,000 BCE it was Thuban in the constellation Ursa Minor. Today Polaris is the last star in the 'tail' of Ursa Minor.

Note 2

'Sun time' and 'clock time' are different. Sun time is based on the fact that the sun reaches its highest point (the meridian), in the middle of the day, and on the next day at its highest point, it will have completed a full cycle. However, the time between the sun reaching successive meridians is often different from clock time. According to clock time, from May to August, the day is close to 24 hours, but in late October the days are about 15 minutes shorter, while in mid February the days are about 14 minutes longer. For our daily routines, it is important to have a constant 'clock time' of 24 hours. This variation is called the 'Equation of Time' and shows the relationship between sun time and clock time. The variation has two causes; the plane of the Earth's equator is inclined to the Earth's orbit around the Sun, and the orbit of the Earth around the sun is an ellipse and not a circle. The National Maritime Museum website shows two separate graphs for these causes, and a third graph where they are combined to give the full correction.

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Kara Holsopple
Host/Producer

Kara Holsopple is committed to telling environmental stories that connect people to faces and places nearby, and to the wider world. Kara is a lifelong resident of southwestern Pennsylvania, except for her undergraduate years at Sarah Lawrence College. She holds a masters degree in professional writing from Chatham University, and has been a features writer for regional magazines. Kara got her start in radio working with Pittsburgh Indymedia’s Rustbelt Radio. She produced "The Allegheny Front Rewind" series, celebrating the show's 20th anniversary, and her work has been heard on The Environment Report, Inside Appalachia and Here Now. One summer she read all of Agatha Christie’s detective novels.

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