images of Haumea were recorded as early as 1955 at the
Palomar Observatory On December 28, 2004, Mike Brown and his team discovered Haumea on images they had taken with the 1.3 m SMARTS Telescope from the
Cerro Tololo Inter-American Observatory in
Chile at the
Palomar Observatory in the
United States on May 6, 2004, while looking for what he hoped would be the
tenth planet. The Caltech discovery team used the nickname "
Santa" among themselves, because they had discovered Haumea on December 28, 2004, just after
Christmas. However, it was clearly too small to be a planet, because it was significantly smaller than
Pluto, and Brown did not announce the discovery. Instead he kept it under wraps, along with several other large
trans-Neptunian objects (TNOs), pending additional observation to better determine their natures. When his team discovered
Haumea's moons, they realized that Haumea was more
rocky than other TNOs, and that its moons were mostly ice. On July 7, 2005, while he was finishing the paper describing the discovery, Brown's daughter Lilah was born, which delayed the announcement further. On July 20, the Caltech team published an online abstract of a report intended to announce the discovery at a conference the following September. In this Haumea was given the code K40506A. At around that time, Pablo Santos Sanz, a student of
José Luis Ortiz Moreno at the
Instituto de Astrofísica de Andalucía at
Sierra Nevada Observatory in southern Spain, claims to have examined the backlog of photos that the Ortiz team had started taking in December 2002. He says that he found Haumea in late July 2005, on images taken on March 7, 9, and 10, 2003. He further said that in checking whether this was a known object, the team came across Brown's internet summary, describing a bright TNO much like the one they had just found.
Googling the reference number for object K40506A on the morning of July 26, they found the Caltech observation logs of Haumea, but according to their account, those logs contained too little information for Ortiz to tell if they were the same object. The Ortiz team also checked with the
Minor Planet Center (MPC), which had no record of this object. Wanting to establish priority, they emailed the MPC with their discovery on the night of July 27, 2005, titled "Big TNO discovery, urgent", without making any mention of the Caltech logs. The next morning they again accessed the Caltech logs, including observations from several additional nights. They then asked Reiner Stoss at the amateur Astronomical Observatory of
Mallorca for further observations. Stoss found
precovery images of Haumea in digitized
Palomar Observatory slides from 1955, and located Haumea with his own telescope that night, July 28. Within an hour, The data was published by the MPC on July 29. On July 29, 2005, Haumea was given its first official label, the temporary designation 2003 EL61, with the "2003" based on the date of the Spanish discovery image. On September 7, 2006, it was numbered and admitted into the official minor planet catalogue as (136108) 2003 EL61. ==Reaction to the announcement==